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Dark Nebula in Scorpio - A dark cloud in Scorpius - Unnamed nebula in Scorpius....

Dark Nebula in Scorpio - A dark cloud in Scorpius - Unnamed nebula in Scorpius. Bright rimmed globules and the
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Largest available format 3978 × 2632 px 4 MB
Dimension [pixels] Dimension in 300dpi [mm] File size [MB] Online Purchase
Large 3978 × 2632 px 337 × 223 mm 4.0 MB
Medium 1024 × 678 px 87 × 57 mm 1.5 MB

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IMAGE number
PIX4621601
Image title
Dark Nebula in Scorpio - A dark cloud in Scorpius - Unnamed nebula in Scorpius. Bright rimmed globules and their more evolved cousin the cometary globule represent fascinating dynamic structures formed by the interplay of cold molecular clouds and hot ionizing stars. Typically the head of the globule faces a hot O - type star. Intense radiation from the star boils away lower density gas from the head. The evaporated rim of gas becomes ionized by the stars ultraviolet flux forming a bright glowing rim we associate with many of these globules including CG4. Intense stellar winds from the ionizing star evaporate gas and dust away from the head forming the “” tail”” and completing the cometary shape. The blood cells are known to be the birthplace of low mass stars. Stars form within the blood cells by the mechanism known as “” radiation driven implosion”. This process occurs when ultraviolet flux from a hot star compresses surviving clumps of cold molecular gas eventually causing collapse and core formation within the dense compact clouds. Lower and intermediate mass stars ultimately form from the compact gas and dust within the blood cells
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Dark Nebula in Scorpio - A dark cloud in Scorpius - Unnamed nebula in Scorpius. Bright rimmed globules and their more evolved cousin the cometary globule represent fascinating dynamic structures formed by the interplay of cold molecular clouds and hot ionizing stars. Typically the head of the globule faces a hot O - type star. Intense radiation from the star boils away lower density gas from the head. The evaporated rim of gas becomes ionized by the stars ultraviolet flux forming a bright glowing rim we associate with many of these globules including CG4. Intense stellar winds from the ionizing star evaporate gas and dust away from the head forming the “” tail”” and completing the cometary shape. The blood cells are known to be the birthplace of low mass stars. Stars form within the blood cells by the mechanism known as “” radiation driven implosion”. This process occurs when ultraviolet flux from a hot star compresses surviving clumps of cold molecular gas eventually causing collapse and core formation within the dense compact clouds. Lower and intermediate mass stars ultimately form from the compact gas and dust within the blood cells

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© R.Gendler/Novapix / Bridgeman Images
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photography / Novapix

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