Sh2-223, Sh2-224, Sh2-225 & Sh2-227 in Auriga (Jan Scheers)

Celestial hemisphere: Northern · Constellation: Auriga (Aur) · Contains: 11 Aur) · 11 mu. Aur · 15 Aur) · 15 lam Aur · 20 Aur · 20 rho Aur · IC 406 · LBN 768 · LBN 769 · LBN 778 · LBN 781 · NGC 1857 · Sh2-223 · Sh2-224 · Sh2-225 · Sh2-227 · The star Alhiba I (μ Aur · The star Alhiba II (λ Aur · The star ρ Aur

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Sh2-223, Sh2-224, Sh2-225 & Sh2-227 in Auriga

Link: http://www.nachthemel.be/Sh2-224.html

Powered byPixInsight

Sh2-223, Sh2-224, Sh2-225 & Sh2-227 in Auriga

Link: http://www.nachthemel.be/Sh2-224.html

SHO-image of Sharpless 223, 224, 225 and 227 in the constellation Auriga.

Sh2-224 is a very faint supernova remnant at distance of about 14700 light years (in the Perseus arm of the Milky Way).
Sh2-223, Sh2-225 and Sh2-227 are faint emission nebulae, H II regions.

This SHO-image is acquired with the Takahashi FSQ-106ED refractor and FLI PL16803 camera from Telescope Live in IC Astronomy Observatory, Oria, Spain.

Total integration time 360 minutes
SHO: 12 sub-frames of 600s with each narrowband filter.
Dataset Telescope Live.

Processing with PixInsight (using AutoIntegrate script), StaXTerminator, Photoshop CC with AstroPanel Pro, Astronomy Tools, Topaz Sharpen AI and NoiseXTerminator plug-ins.

Sharpless2 Objects
Southern Hemisphere Astro
Telescope.live
Narrowband imaging

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Status	Advanced success
Started	...
Astrometry.net job	6616372
PixInsight job	CTBENNXCSOCQ6GUN0845ZKK9Q2G2SJZT
PixInsight queue size	n/a
PixInsight stage	TASK_LOG

RA (center)	05h23m15s.11
RA (top/left)	05h06m55s.83
RA (top/right)	05h12m19s.78
RA (bottom/right)	05h38m32s.63
RA (bottom/left)	05h35m11s.22

Dec (center)	+41°01′38″.9
Dec (top/left)	+43°04′43″.8
Dec (top/right)	+38°02′01″.5
Dec (bottom/right)	+38°50′28″.1
Dec (bottom/left)	+43°56′55″.9

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Sh2-223, Sh2-224, Sh2-225 & Sh2-227 in Auriga

Sh2-223, Sh2-224, Sh2-225 & Sh2-227 in Auriga

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Image Index:

Contribution Index (beta):

Sh2-223, Sh2-224, Sh2-225 & Sh2-227 in Auriga

Sh2-223, Sh2-224, Sh2-225 & Sh2-227 in Auriga

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