LDN 1622 - Bogeyman Nebula (Alexkid)

Celestial hemisphere: Northern · Constellation: Orion (Ori) · Contains: 56 Ori · LDN 1621 · LDN 1622 · LDN 1624 · The star 56Ori · VdB62 · VdB63

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LDN 1622 - Bogeyman Nebula

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LDN 1622 - Bogeyman Nebula

French Version

LDN 1622 et LDN 1621 sont une paire de nébuleuses sombres qui se trouvent devant une vaste zone de nébulosité d'émission qui fait partie de la boucle de Barnard au centre d'Orion. Cette zone fait partie du nuage moléculaire Orion beaucoup plus grand.
On pense qu'ils sont situés à 500 années-lumière de nous. Ce complexe de nébulosité sombre est parfois appelé la nébuleuse Bogeyman, bien qu'il existe plusieurs orthographes différentes, notamment Boogeyman, Bogey Man, Boogey Man, Boogieman et Boogie Man. Elle est aussi parfois appelée la nébuleuse du Fantôme. Ces nébuleuses ont été cataloguées par Beverly T. Lynds en 1962.

English Version

LDN 1622 and LDN 1621 are a pair of dark nebulae that lie in front of a large area of emission nebulosity that is part of the Barnard's Loop in central Orion. This area is part of the much larger Orion molecular cloud.
They are believed to be located 500 light years from us. This complex of dark nebulosity is sometimes referred to as the Bogeyman Nebula, although there are several different spellings, including Boogeyman, Bogey Man, Boogey Man, Boogieman, and Boogie Man. It is also sometimes called the Ghost Nebula. These nebulae were cataloged by Beverly T. Lynds in 1962.

Données gratuites Deep Sky West
instrument : Takahashi FSQ 130
L : 25 x 900s
R : 15 x 900s
G : 23 x 900s
B : 11 x 900s
Halpha : 28 x 1800s

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Status	Advanced success
Started	...
PixInsight job	V91RE1KK97KHFJ6N4NTOQBR9IM90FB5P
PixInsight queue size	n/a
PixInsight stage	TASK_LOG

RA (center)	05h54m44s.16
RA (top/left)	05h51m48s.83
RA (top/right)	05h51m55s.26
RA (bottom/right)	05h57m39s.81
RA (bottom/left)	05h57m34s.13

Dec (center)	+02°02′07″.9
Dec (top/left)	+02°59′09″.5
Dec (top/right)	+01°04′08″.8
Dec (bottom/right)	+01°05′05″.9
Dec (bottom/left)	+03°00′10″.4

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