Celestial hemisphere:  Northern  ·  Constellation: Orion (Ori)  ·  Contains:  NGC 2112  ·  The star 56Ori  ·  The star 59Ori  ·  The star 60Ori
The Boogieman, Rutger Bus
The Boogieman
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The Boogieman, Rutger Bus
The Boogieman
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Description

Yesterday I was able to shoot 5h of data with my Omegon RC6", Ha-filter and ASI1600MM camera on the BoogieMan nebula. I combined this data with Duo-Band data (2h) which I shot last year with William Optics GT71 and ASI294MC pro camera to get more details in the dark dust areas. Hope you like it.

The Boogie Man Nebula (also known as Lynds’ Dark Nebula (LDN) 1622) is a dark molecular cloud of less than 10 light-years across that lies only 500 light-years away in the constellation of Orion, close on the sky to Barnard’s Loop and just north of Orion’s belt, near the plane of our Milky Way Galaxy.

The BoogieMan Nebula appears against a faint background of glowing hydrogen gas. The interstellar dust of this dark nebula is so thick that it obscures light from nearby stars or other nebulas.

This nebula demonstrates the evolution of stars. Star formation results from the collapse of giant clouds of molecular gas and dust. The stars eventually emerge into visibility.

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The Boogieman, Rutger Bus