Celestial hemisphere:  Northern  ·  Constellation: Cygnus (Cyg)  ·  Contains:  Crescent Nebula  ·  IC 4996  ·  NGC 6888  ·  The star 28Cyg  ·  The star 29Cyg  ·  The star 34Cyg  ·  The star 36Cyg
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NGC 6888, The Crescent Nebula, Paul Kent
NGC 6888, The Crescent Nebula
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NGC 6888, The Crescent Nebula

Getting plate-solving status, please wait...
NGC 6888, The Crescent Nebula, Paul Kent
NGC 6888, The Crescent Nebula
Powered byPixInsight

NGC 6888, The Crescent Nebula

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Description

The Crescent Nebula is formed from strong stellar outflows from the central star. This star is a Wolf Rayet type, similar to the bubble nebula. It is a very massive, very hot star that has become unstable after its evolution on the main sequence. This is specifically WR136, which has a surface temp of 71,000K, over 10x hotter than the sun. This makes the star incredibly luminous, and supplies the energy required to ionise the gas it threw off. These shells of ionised gas are clearly seen surrounding the star. The electric blue colour here shows that the O3 emission is high compared to most other nebulae where it is usually much weaker than Ha. In contrast to the strong O3, the S2 emission is almost non -existant for the Crescent itself. It however is present in enough quantity in the surrounding 'field' gas to show through and a rusty colour.

Also present near the top centre is small, asymmetric Planetary Nebula, Abell 69.

In the upper left, the round nebula is SH2-104 from the Sharpless catalogue.

And that red star next to the crescent sticks out like a sore thumb. A bit of investigating shows it to be RS Cygni...not only a variable, but a Carbon star. These are very red due to carbon absorbing blue light.

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NGC 6888, The Crescent Nebula, Paul Kent