M27

 

OBJECT: Messier27


This is the wellknown planetary nebula in Vulpecula. It is about 8 arcminutes wide and fairly bright at magnitude 7.5. The central star is a white dwarf. In the central region of the nebula one can find a "pattern of dark and bright cusped knots". They are best seen in H-alpha against the O-III abundant teal-colored gas.

There are faint wisps visible around the outer regions, which show up at long exposures and with image process enhancements.


I made exposures in L, R, G, B, S, H and O. Here I present the nebula in an HOO-blended version (greenish-blue) as well as a more normal RGB version (more greenish appearance). 

OBJECT

M27 or NGC6853

Vulpecula

OPTICS

12" f/8 1:1 flattener

f.l. 2432mm

FILTERS

Ha 3.5nm + OIII 4nm + SII 4nm + LRGB

-

CAMERA

QHY600M PH

BIN2. 0.6"/pixel

EXPOSURE

Ha: 9x5min

OIII: 9x5min

SII 9x5min

LRGB: 6x3min each

SHO: 2h 15min

LRGB: 1h 12min

Tot: 3h 27min

PROCESSING

Maxim DL / Pixinsight

BlurXT NoiseXT

COLOUR Scheme

LRGBSHO blended

HOO "blue enhanced" blended with LRGB+S

DATE

2025-08-26

-

OBJECT

M27 or NGC6853

Vulpecula

OPTICS

12" f/8 1:1 flattener

f.l. 2432mm

FILTERS

Ha 3.5nm + OIII 4nm + SII 4nm +LRGB

-

CAMERA

QHY600M PH

BIN2. 0.6"/pixel

EXPOSURE

Ha: 9x5min

OIII: 9x5min

SII: 9x5min

LRGB: 6x3min each

SHO 2h 15min

LRGB: 1h 12min

Tot: 3h 27min

PROCESSING

Maxim DL / Pixinsight

BlurXT NoiseXT

Local Histogram Eq etc

COLOUR Scheme

LRGBSHO

"Normal" RGB

DATE

2025-08-26

-