NGC2174

 

OBJECT: NGC2174 (Sh2-252, LBN854, IC2159)


This emission nebula in northern Orion is sometimes called the Monkey Head Nebula. It is associated with the open star cluster NGC2175. It has rather good emission in both S-II, Ha and O-III. It was discovered by Edouard Stephan on Feb 6 1877, the same year as he discovered what is now called Stephans quintet. (The designations 2174 and 2175 are sometimes used the other way around.)

In the center we see bluish hot gas. Young hot blue stars generate stellar winds and high energy radiation transforming regions of the surrounding gas into clumps and possible stellar creation.

I made exposures over 2 nights in S, H and O. The bright star in the middle is the O6-star HD42088 at magnitude 7.6.

Here I present the nebula in HOO and SHO representations. All image files are dark and flat field corrected. North is to the right.

OBJECT

NGC2174

Orion

OPTICS

12" f/8 RC

f.l. 2432mm

FILTERS

Ha 3.5nm + OIII 4nm

-

CAMERA

QHY600M PH

BIN2 0.6"/pixel

EXPOSURE

Ha: 15x5min

OIII: 14x5min

Tot: 2h 25min

PROCESSING

Maxim DL / Pixinsight

BlurXT NoiseXT

COLOUR Scheme

HOO as RGB

-

DATE

2024-11-22, 28

-

OBJECT

NGC2174

Orion

OPTICS

12" f/8 RC

f.l. 2432mm

FILTERS

Ha 3.5nm + OIII 4nm + SII 4nm

-

CAMERA

QHY600M PH

BIN2 0.6"/pixel

EXPOSURE

Ha: 15x5min

OIII: 14x5min

SII: 14x5min

Tot: 3h 35min

PROCESSING

Maxim DL / Pixinsight

BlurXT NoiseXT

COLOUR Scheme

H-SHO as L-RGB

-

DATE

2024-11-22, 28

-