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Barbara Bouchet at Canzonissima

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Ela Weber presenting the TV broadcast Tira & Molla, Rome, Italy

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Television screen displaying a simulation of John Glenn in the Friendship 7 space capsule. There were no publicly broadcast images of Glenn during the first US orbital space flight. February 20, 1962

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Television screen displaying a simulation of John Glenn in the Friendship 7 space capsule. There were no publicly broadcast images of Glenn during the first US orbital space flight. February 20, 1962

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Italian TV host Pippo Baudo with comedy trio 'La Smorfia', Italy, 1979 (b/w photo)

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Italian TV host Pippo Baudo with comedy trio 'La Smorfia', Italy, 1979 (b/w photo)

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Italian TV host Pippo Baudo with Alida Chelli during the rehearsals for a TV show, Italy, 1975 (b/w photo)

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Italian TV host Pippo Baudo with Alida Chelli during the rehearsals for a TV show, Italy, 1975 (b/w photo)

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XRA2681006

Jean Marie Le Pen

XRA2681006

 
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Jean Marie Le Pen

XRA2681007

Jean Marie Le Pen

XRA2681007

 
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Jean Marie Le Pen et Armand Jammot

XRA2681009

Jean Marie Le Pen et Armand Jammot

XRA2681009

 
Omega nebula (M17) in Sagittarius - The Omega nebula (M17) in Sagittarius - View of the Omega nebula (M17/NGC 6618) located in the constellation Sagittarius at a distance of 5700 light years. This object derives its name from its looped shape reminiscent of the Greek letter when the nebula is seen in a telescope. The gas cloud is unusual in that it does not appear to be illuminated by the bright stars that commonly found in emission nebulae such as this. However, the nebulosity is very bright, so the exciting stars must be hidden within the cloud, an idea confirmed by the infrared brightness of the nebula. As well as exciting the nebula we can see, the embedded stars heat the dust that surrounds them, so M17 is one of the brightest objects in the infrared sky. It is about 6000 light years distant

Adam Block

PIX4620160

Omega nebula (M17) in Sagittarius - The Omega nebula (M17) in Sagittarius - View of the Omega nebula (M17/NGC 6618) located in the constellation Sagittarius at a distance of 5700 light years. This object derives its name from its looped shape reminiscent of the Greek letter when the nebula is seen in a telescope. The gas cloud is unusual in that it does not appear to be illuminated by the bright stars that commonly found in emission nebulae such as this. However, the nebulosity is very bright, so the exciting stars must be hidden within the cloud, an idea confirmed by the infrared brightness of the nebula. As well as exciting the nebula we can see, the embedded stars heat the dust that surrounds them, so M17 is one of the brightest objects in the infrared sky. It is about 6000 light years distant

Adam Block

PIX4620160

 
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Jean Marie Le Pen

XRA2681008

Jean Marie Le Pen

XRA2681008

 
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Carosello's theme

Archivio TV Sorrisi e Canzoni

MEP2388659

Carosello's theme

Archivio TV Sorrisi e Canzoni

MEP2388659

 
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Television screen animation of John Glenn's Friendship 7 space capsule approaching North America, during his three orbit space flight on Feb. 20, 1962

EVB2942026

Television screen animation of John Glenn's Friendship 7 space capsule approaching North America, during his three orbit space flight on Feb. 20, 1962

EVB2942026

 
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Surgery class shooted by the TV, Milan, Italy

MEP2533564

Surgery class shooted by the TV, Milan, Italy

MEP2533564

 
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General de Gaulle broadcasts to the Free French (gouache on paper)

Nicolle, Pat (Patrick) (1907-95)

LAL724099

General de Gaulle broadcasts to the Free French (gouache on paper)

Nicolle, Pat (Patrick) (1907-95)

LAL724099

 
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Herbert George Wells during a speech at the radio (b/w photo)

XRH993861

Herbert George Wells during a speech at the radio (b/w photo)

XRH993861

 
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Paolo Bonolis and Ela Weber at the TV broadcast Tira & Molla, Rome, Italy

Mario Notarangelo

MEP2516240

Paolo Bonolis and Ela Weber at the TV broadcast Tira & Molla, Rome, Italy

Mario Notarangelo

MEP2516240

 
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Jean Marie Le Pen

XRA2681024

Jean Marie Le Pen

XRA2681024

 
Nebula IC 1274 in Sagittariu - Nebula IC 1274 in Sagittariu

Adam Block

PIX4622142

Nebula IC 1274 in Sagittariu - Nebula IC 1274 in Sagittariu

Adam Block

PIX4622142

 
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Jean Marie Le Pen

XRA2681038

Jean Marie Le Pen

XRA2681038

 
Omega nebula (M17) in Sagittarius - The Omega nebula (M17) in Sagittarius - View of the Omega nebula (M17/NGC 6618) located in the constellation Sagittarius at a distance of 5700 light years. This object derives its name from its looped shape reminiscent of the Greek letter when the nebula is seen in a telescope. The gas cloud is unusual in that it does not appear to be illuminated by the bright stars that commonly found in emission nebulae such as this. However, the nebulosity is very bright, so the exciting stars must be hidden within the cloud, an idea confirmed by the infrared brightness of the nebula. As well as exciting the nebula we can see, the embedded stars heat the dust that surrounds them, so M17 is one of the brightest objects in the infrared sky. It is about 6000 light years distant

PIX4620118

Omega nebula (M17) in Sagittarius - The Omega nebula (M17) in Sagittarius - View of the Omega nebula (M17/NGC 6618) located in the constellation Sagittarius at a distance of 5700 light years. This object derives its name from its looped shape reminiscent of the Greek letter when the nebula is seen in a telescope. The gas cloud is unusual in that it does not appear to be illuminated by the bright stars that commonly found in emission nebulae such as this. However, the nebulosity is very bright, so the exciting stars must be hidden within the cloud, an idea confirmed by the infrared brightness of the nebula. As well as exciting the nebula we can see, the embedded stars heat the dust that surrounds them, so M17 is one of the brightest objects in the infrared sky. It is about 6000 light years distant

PIX4620118

 
Omega nebula (M17) in Sagittarius - The Omega nebula (M17) in Sagittarius - View of the Omega nebula (M17/NGC 6618) located in the constellation Sagittarius at a distance of 5700 light years. This object derives its name from its looped shape reminiscent of the Greek letter when the nebula is seen in a telescope. The gas cloud is unusual in that it does not appear to be illuminated by the bright stars that commonly found in emission nebulae such as this. However, the nebulosity is very bright, so the exciting stars must be hidden within the cloud, an idea confirmed by the infrared brightness of the nebula. As well as exciting the nebula we can see, the embedded stars heat the dust that surrounds them, so M17 is one of the brightest objects in the infrared sky. It is about 6000 light years distant

PIX4620153

Omega nebula (M17) in Sagittarius - The Omega nebula (M17) in Sagittarius - View of the Omega nebula (M17/NGC 6618) located in the constellation Sagittarius at a distance of 5700 light years. This object derives its name from its looped shape reminiscent of the Greek letter when the nebula is seen in a telescope. The gas cloud is unusual in that it does not appear to be illuminated by the bright stars that commonly found in emission nebulae such as this. However, the nebulosity is very bright, so the exciting stars must be hidden within the cloud, an idea confirmed by the infrared brightness of the nebula. As well as exciting the nebula we can see, the embedded stars heat the dust that surrounds them, so M17 is one of the brightest objects in the infrared sky. It is about 6000 light years distant

PIX4620153

 
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Switzerland Television Demonstration Eth (b/w photo)

Stringer (STR)

KES6253618

Switzerland Television Demonstration Eth (b/w photo)

Stringer (STR)

KES6253618

 
Omega nebula (M17) in Sagittarius - The Omega nebula (M17) in Sagittarius - View of the Omega nebula (M17/NGC 6618) located in the constellation Sagittarius at a distance of 5700 light years. Image obtained by the VST (VLT Survey Telescope) in Chile in June 2011. The first released VST image shows the spectacular star - forming region Messier 17, also known as the Omega Nebula or the Swan Nebula, as it has never been seen before. This vast region of gas, dust and hot young stars lies in the heart of the Milky Way in the constellation of Sagittarius (The Archer). The VST field of view is so large that the entire nebula, including its fainter outer parts, is captured - - and retains its superb sharpness across the entire image

PIX4620192

Omega nebula (M17) in Sagittarius - The Omega nebula (M17) in Sagittarius - View of the Omega nebula (M17/NGC 6618) located in the constellation Sagittarius at a distance of 5700 light years. Image obtained by the VST (VLT Survey Telescope) in Chile in June 2011. The first released VST image shows the spectacular star - forming region Messier 17, also known as the Omega Nebula or the Swan Nebula, as it has never been seen before. This vast region of gas, dust and hot young stars lies in the heart of the Milky Way in the constellation of Sagittarius (The Archer). The VST field of view is so large that the entire nebula, including its fainter outer parts, is captured - - and retains its superb sharpness across the entire image

PIX4620192

 
Nebula near the star S Mon in Unicorn - Fox Fur nebula in Monoceros - Nebula around the bright star S Monocerotis in the constellation Unicorn. S My belongs to a young cluster of stars located about 2600 years from Earth. The region around the 4.7 magnitude star S Mon is a fascinating mixture of red fluorescent hydrogen and dark, obscuring dust lanes. Some dust patches are close enough to bright stars to reflect light from them; these appear blue for the same reason that the day - time sky is blue - because some of the interstellar particles preferentially scatter blue light. The dust is mixed with gas and this affects the appearance of the emission nebulae, giving some of the faintest a curious 'fox fur' texture in this enhanced photograph. S Mon is part of a young open cluster of stars named NGC 2264 located about 2600 light years away, just north of the Cone nebula

PIX4618692

Nebula near the star S Mon in Unicorn - Fox Fur nebula in Monoceros - Nebula around the bright star S Monocerotis in the constellation Unicorn. S My belongs to a young cluster of stars located about 2600 years from Earth. The region around the 4.7 magnitude star S Mon is a fascinating mixture of red fluorescent hydrogen and dark, obscuring dust lanes. Some dust patches are close enough to bright stars to reflect light from them; these appear blue for the same reason that the day - time sky is blue - because some of the interstellar particles preferentially scatter blue light. The dust is mixed with gas and this affects the appearance of the emission nebulae, giving some of the faintest a curious 'fox fur' texture in this enhanced photograph. S Mon is part of a young open cluster of stars named NGC 2264 located about 2600 light years away, just north of the Cone nebula

PIX4618692

 
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William Joyce (Lord Haw Haw) (gouache on paper)

Nicolle, Pat (Patrick) (1907-95)

LAL724102

William Joyce (Lord Haw Haw) (gouache on paper)

Nicolle, Pat (Patrick) (1907-95)

LAL724102

 
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Jean Marie Le Pen

XRA2681046

Jean Marie Le Pen

XRA2681046

 
Centre de la nebula de la Lagoon (M8) dans le Sagittarius - In the heart of the Lagoon Nebula - Centre de la nebula de la Lagoon (M8) vue par le telescope Hubble (HST). This close - up shot of the centre of the Lagoon Nebula (Messier 8) clearly shows the delicate structures formed when the powerful radiation of young stars interacts with the hydrogen cloud they formed from. This image was created from exposures taken with the Wide Field Channel of the Advanced Camera for Surveys on Hubble. Light from glowing hydrogen (through the F658N filter) is coloured red. Light from ionised nitrogen (through the F660N filter) is coloured green and light through a yellow filter (F550M) is coloured blue. The exposure times through each filter are 1560 s, 1600 s and 400 s respectively. The blue - white flare at the upper - left of the image is scattered light from a bright star just outside the field of view. The field of view is about 3.3 by 1.7 arcminutes

PIX4619692

Centre de la nebula de la Lagoon (M8) dans le Sagittarius - In the heart of the Lagoon Nebula - Centre de la nebula de la Lagoon (M8) vue par le telescope Hubble (HST). This close - up shot of the centre of the Lagoon Nebula (Messier 8) clearly shows the delicate structures formed when the powerful radiation of young stars interacts with the hydrogen cloud they formed from. This image was created from exposures taken with the Wide Field Channel of the Advanced Camera for Surveys on Hubble. Light from glowing hydrogen (through the F658N filter) is coloured red. Light from ionised nitrogen (through the F660N filter) is coloured green and light through a yellow filter (F550M) is coloured blue. The exposure times through each filter are 1560 s, 1600 s and 400 s respectively. The blue - white flare at the upper - left of the image is scattered light from a bright star just outside the field of view. The field of view is about 3.3 by 1.7 arcminutes

PIX4619692

 
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JUBILEE BROADCAST to US Troops, Aug.1945.Count Basie (piano)Illinois Jacquet(sax)Tommy Dorsey, Ziggy Elman, Buddy Rich, Artie Shaw, Lionel Hampton(vibes)

EVB2949926

JUBILEE BROADCAST to US Troops, Aug.1945.Count Basie (piano)Illinois Jacquet(sax)Tommy Dorsey, Ziggy Elman, Buddy Rich, Artie Shaw, Lionel Hampton(vibes)

EVB2949926

 
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United States, 1960s: College graduation ceremony

AVE6321377

United States, 1960s: College graduation ceremony

AVE6321377

 
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Sergio Zavoli interviewing some racing cyclists, Sanremo, Italy, 1968

Giorgio Lotti

MEP2338068

Sergio Zavoli interviewing some racing cyclists, Sanremo, Italy, 1968

Giorgio Lotti

MEP2338068

 
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Marco Giusti with a blob on his face, Italy

Rino Petrosino

MEP2516224

Marco Giusti with a blob on his face, Italy

Rino Petrosino

MEP2516224

 
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Bluebell Girls dancers in the dressing rooms, Italy, 1961 (b/w photo)

Reporters Associati & Archivi

MEP2829257

Bluebell Girls dancers in the dressing rooms, Italy, 1961 (b/w photo)

Reporters Associati & Archivi

MEP2829257

 
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Radio communications

English School, (20th century)

LAL320097

Radio communications

English School, (20th century)

LAL320097

 
Detail of the Cone nebula in the Unicorn - The Cone Nebula (NGC 2264) - Detail - Image obtained by the Hubble space telescope of the upper part of the Cone nebula (NGC 2264), a star-forming region located about 2500 years ago - light from Earth. The Cone Nebula (NGC 2264) - - so named because, in ground - based images, it has a conical shape - - this giant pillar resides in a turbulent star - forming region. This picture, taken by the Advanced Camera for Surveys (ACS) aboard Nasa's Hubble Space Telescope, shows the upper 2.5 light - years of the nebula, a height that equals 23 million roundtrips to the Moon. The entire nebula is 7 light - years long. The Cone Nebula resides 2,500 light - years away in the constellation Monoceros. ACS made this observation on April 2, 2002. The color image is constructed from three separate images taken in blue, near - infrared, and hydrogen - alpha filters

PIX4618668

Detail of the Cone nebula in the Unicorn - The Cone Nebula (NGC 2264) - Detail - Image obtained by the Hubble space telescope of the upper part of the Cone nebula (NGC 2264), a star-forming region located about 2500 years ago - light from Earth. The Cone Nebula (NGC 2264) - - so named because, in ground - based images, it has a conical shape - - this giant pillar resides in a turbulent star - forming region. This picture, taken by the Advanced Camera for Surveys (ACS) aboard Nasa's Hubble Space Telescope, shows the upper 2.5 light - years of the nebula, a height that equals 23 million roundtrips to the Moon. The entire nebula is 7 light - years long. The Cone Nebula resides 2,500 light - years away in the constellation Monoceros. ACS made this observation on April 2, 2002. The color image is constructed from three separate images taken in blue, near - infrared, and hydrogen - alpha filters

PIX4618668

 
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Wim Thoelke with audience, 1971 (b/w photo)

Alfred Strobel

SZT6304804

Wim Thoelke with audience, 1971 (b/w photo)

Alfred Strobel

SZT6304804

 
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Bluebell Girls rehearsing, Italy, 1961 (b/w photo)

Reporters Associati & Archivi

MEP2834775

Bluebell Girls rehearsing, Italy, 1961 (b/w photo)

Reporters Associati & Archivi

MEP2834775

 
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Italian TV host Pippo Baudo with Heather Parisi during the reharsals for a tv show, Italy, 1984 (b/w photo)

Reporters Associati & Archivi

MEP3111909

Italian TV host Pippo Baudo with Heather Parisi during the reharsals for a tv show, Italy, 1984 (b/w photo)

Reporters Associati & Archivi

MEP3111909

 
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Al Bano and Rita dalla Chiesa, Italy

Rino Petrosino

MEP2514854

Al Bano and Rita dalla Chiesa, Italy

Rino Petrosino

MEP2514854

 
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Barbara Bouchet with Pippo Baudo

Archivio TV Sorrisi e Canzoni

MEP2387406

Barbara Bouchet with Pippo Baudo

Archivio TV Sorrisi e Canzoni

MEP2387406

 
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Luca Barbarossa awarded at 42nd Sanremo Music Festival

Egizio Fabbrici

MEP2382235

Luca Barbarossa awarded at 42nd Sanremo Music Festival

Egizio Fabbrici

MEP2382235

 
Nebula NGC 6559 in Sagittarius - NGC 6559 and IC 1274 - 75 in Sagittarius - Located in Sagittarius, this nebula is located at a distance of about 5000 years - light from Earth. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. This dusty region is probably associated with the brighter and better - known Lagoon and Trifid Nebulae which are nearby in the sky and part of the same molecular cloud. The soft red glow of fluorescent hydrogen is evidence that there are young hot stars associated with the dusty clouds. These bright stars also illuminate the tiny solid particles, producing blue reflection nebulae bordering some of the emission regions. The dust is also evident in silhouette, both as sinuous dark lanes winding through the luminous gas and as the dark patches obscuring the ancient, yellow stars that populate the central parts of the Milky Way

PIX4619800

Nebula NGC 6559 in Sagittarius - NGC 6559 and IC 1274 - 75 in Sagittarius - Located in Sagittarius, this nebula is located at a distance of about 5000 years - light from Earth. Image made with the 1.2m Telescope of Schmidt UK from Siding Spring. This dusty region is probably associated with the brighter and better - known Lagoon and Trifid Nebulae which are nearby in the sky and part of the same molecular cloud. The soft red glow of fluorescent hydrogen is evidence that there are young hot stars associated with the dusty clouds. These bright stars also illuminate the tiny solid particles, producing blue reflection nebulae bordering some of the emission regions. The dust is also evident in silhouette, both as sinuous dark lanes winding through the luminous gas and as the dark patches obscuring the ancient, yellow stars that populate the central parts of the Milky Way

PIX4619800

 
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Bluebell Girls rehearsing, Italy, 1961 (b/w photo)

Reporters Associati & Archivi

MEP2829253

Bluebell Girls rehearsing, Italy, 1961 (b/w photo)

Reporters Associati & Archivi

MEP2829253

 
Microphone, Switzerland (photo)

GNG3957191

Microphone, Switzerland (photo)

GNG3957191

 
Think Kwaito, think Yfm (photo)

UIG2619391

Think Kwaito, think Yfm (photo)

UIG2619391

 
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Bluebell Girls dancer in the dressing rooms, Italy, 1961 (b/w photo)

Reporters Associati & Archivi

MEP2829255

Bluebell Girls dancer in the dressing rooms, Italy, 1961 (b/w photo)

Reporters Associati & Archivi

MEP2829255

 
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Fredy Quinn in the TV show 3x9, 1971 (b/w photo)

Alfred Strobel

SZT6304789

Fredy Quinn in the TV show 3x9, 1971 (b/w photo)

Alfred Strobel

SZT6304789

 
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Dan Blocker in the TV show 3x9, 1971 (b/w photo)

Alfred Strobel

SZT6304779

Dan Blocker in the TV show 3x9, 1971 (b/w photo)

Alfred Strobel

SZT6304779

 
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Orchestra leader JOHN SCOTT TROTTER and BING CROSBY go over lyrics for "Home on the Range" and "The Caissons Go Rolling Along" - requested by General MacArthur for broadcast to the Philippines, 1/29/42

EVB2949620

Orchestra leader JOHN SCOTT TROTTER and BING CROSBY go over lyrics for "Home on the Range" and "The Caissons Go Rolling Along" - requested by General MacArthur for broadcast to the Philippines, 1/29/42

EVB2949620

 
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Switzerland Circus Knee, 1978 (b/w photo)

Stringer (STR)

KES6213283

Switzerland Circus Knee, 1978 (b/w photo)

Stringer (STR)

KES6213283

 
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Lorella Cuccarini talking to Enrico Ruggeri

Rino Petrosino

MEP2382194

Lorella Cuccarini talking to Enrico Ruggeri

Rino Petrosino

MEP2382194

 
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Sergio Zavoli interviewing some racing cyclists, Sanremo, Italy, 1968

Giorgio Lotti

MEP2338061

Sergio Zavoli interviewing some racing cyclists, Sanremo, Italy, 1968

Giorgio Lotti

MEP2338061

 
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Bluebell Girls dancers in the dressing rooms, Italy, 1961 (b/w photo)

Reporters Associati & Archivi

MEP2829259

Bluebell Girls dancers in the dressing rooms, Italy, 1961 (b/w photo)

Reporters Associati & Archivi

MEP2829259

 
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Wim Thoelke and Dan Blocker, 1971 (b/w photo)

Alfred Strobel

SZT6304778

Wim Thoelke and Dan Blocker, 1971 (b/w photo)

Alfred Strobel

SZT6304778

 
Nebula Trifide (M20) in the constellation Sagittarius - Trifid nebula (M20) in Sagittarius - View of the center of the Trifide nebula (M20/NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 years - light from Earth. Image obtained by Siding Spring's 3.9m telescope. Vast clouds of hydrogen mixed with tiny dust grains are distributed throughout the Milky Way. The hydrogen can only be seen at visible wavelengths when it is illuminated by very hot stars. The light from these stars is sufficiently rich in ultraviolet light to cause the gas to glow with its characteristic red colour. In most cases, such as here, the hot stars formed recently from the hydrogen cloud. The stars found at the heart of the Trifid Nebula are here seen associated with dust lanes which are silhouetted against the glowing background. This nebula is in the constellation of Sagittarius at a distance between 5000 and 10,000 light years

PIX4619647

Nebula Trifide (M20) in the constellation Sagittarius - Trifid nebula (M20) in Sagittarius - View of the center of the Trifide nebula (M20/NGC 6514) located in the constellation Sagittarius between 5000 and 10,000 years - light from Earth. Image obtained by Siding Spring's 3.9m telescope. Vast clouds of hydrogen mixed with tiny dust grains are distributed throughout the Milky Way. The hydrogen can only be seen at visible wavelengths when it is illuminated by very hot stars. The light from these stars is sufficiently rich in ultraviolet light to cause the gas to glow with its characteristic red colour. In most cases, such as here, the hot stars formed recently from the hydrogen cloud. The stars found at the heart of the Trifid Nebula are here seen associated with dust lanes which are silhouetted against the glowing background. This nebula is in the constellation of Sagittarius at a distance between 5000 and 10,000 light years

PIX4619647

 
The Lagoon nebula (M8) without stars - The Lagoon nebula (M8) with stars removed - In this image, the stars were removed by computer processing. Located in Sagittarius, at a distance of 5800 years - light, M8 is visible to the naked eye in good conditions. It is a star-forming region illuminated by several large O-type stars that belong to the open cluster NGC 6530 visible in the center of the image. The brightest part of the nebula is called the hourglass nebula whose gases are excited mainly by two massive supergeant stars Herschel 36 and 9 Sagittarii. M8 has at least 60 Giant B stars, 3 to 4 times more than the Orion Nebula. This image was processed to remove the stars so the incredible complex of dark and light nebulosity could more easily be seen. M8 is an amazing stellar nursery. Hot young stars that formed out of the hydrogen gas in the nebula cause it to glow in the light of ionized hydrogen at the hydrogen - alpha wavelength of 656nm. The Lagoon Nebula gets its name from the d

Jerry Lodriguss

PIX4619678

The Lagoon nebula (M8) without stars - The Lagoon nebula (M8) with stars removed - In this image, the stars were removed by computer processing. Located in Sagittarius, at a distance of 5800 years - light, M8 is visible to the naked eye in good conditions. It is a star-forming region illuminated by several large O-type stars that belong to the open cluster NGC 6530 visible in the center of the image. The brightest part of the nebula is called the hourglass nebula whose gases are excited mainly by two massive supergeant stars Herschel 36 and 9 Sagittarii. M8 has at least 60 Giant B stars, 3 to 4 times more than the Orion Nebula. This image was processed to remove the stars so the incredible complex of dark and light nebulosity could more easily be seen. M8 is an amazing stellar nursery. Hot young stars that formed out of the hydrogen gas in the nebula cause it to glow in the light of ionized hydrogen at the hydrogen - alpha wavelength of 656nm. The Lagoon Nebula gets its name from the d

Jerry Lodriguss

PIX4619678

 
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Roberto Villa, Corrado, Gino Bramieri, Marida Del Frate and Raffaele Pisu in the variety show 'L'amico del Giaguaro'

Archivio TV Sorrisi e Canzoni

MEP2380715

Roberto Villa, Corrado, Gino Bramieri, Marida Del Frate and Raffaele Pisu in the variety show 'L'amico del Giaguaro'

Archivio TV Sorrisi e Canzoni

MEP2380715

 
Nebula NGC 3372 in the Carene - The Carina nebula, NGC 3372 - The Carene nebula is located about 7000 years from the Earth. It is home to many hot stars, including the star Eta Carinae in the centre of the nebula. Image obtained by Siding Spring's 3.9m telescope. The brightest part of the Milky Way, as seen by the unaided eye, lies in the southern constellation Carina. Here there are an unusually large number of young, hot stars. Their radiation is rich in energetic ultraviolet light. Many of these stars were born within the spectacular Carinae nebula, seen here. The nebula is a cloud of glowing gas composed mostly of hydrogen. It excited by ultrviolet light from the embedded stars. This dostictive emission radiation is responsible for the red colour. About a quarter of the nebula is made of helium gas, the second most abundant element in the universe after hydrogen, and all the other chemical elements account for only a few percent of the total mass. The brightest star in the nebula i

PIX4618887

Nebula NGC 3372 in the Carene - The Carina nebula, NGC 3372 - The Carene nebula is located about 7000 years from the Earth. It is home to many hot stars, including the star Eta Carinae in the centre of the nebula. Image obtained by Siding Spring's 3.9m telescope. The brightest part of the Milky Way, as seen by the unaided eye, lies in the southern constellation Carina. Here there are an unusually large number of young, hot stars. Their radiation is rich in energetic ultraviolet light. Many of these stars were born within the spectacular Carinae nebula, seen here. The nebula is a cloud of glowing gas composed mostly of hydrogen. It excited by ultrviolet light from the embedded stars. This dostictive emission radiation is responsible for the red colour. About a quarter of the nebula is made of helium gas, the second most abundant element in the universe after hydrogen, and all the other chemical elements account for only a few percent of the total mass. The brightest star in the nebula i

PIX4618887

 
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Director's meeting in the Nuernberger Funkhaus, 1937 (b/w photo)

SZT2984284

Director's meeting in the Nuernberger Funkhaus, 1937 (b/w photo)

SZT2984284

 
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Director's meeting in the Nuernberger Funkhaus, 1937 (b/w photo)

SZT2984295

Director's meeting in the Nuernberger Funkhaus, 1937 (b/w photo)

SZT2984295

 
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Band in the TV show 3x9, 1971 (b/w photo)

Alfred Strobel

SZT6304793

Band in the TV show 3x9, 1971 (b/w photo)

Alfred Strobel

SZT6304793

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