Large Magellanic Cloud ; NGC 2030 et al (Michelle Bennett)

Celestial hemisphere: Southern · Constellation: Dorado (Dor) · Contains: HD269698 · HD269702 · HD269713 · HD269714 · HD269717 · HD269723 · HD269724 · HD269726 · HD269733 · HD269771 · HD269777 · HD269789 · HD269797 · HD269808 · HD269810 · HD269811 · HD269827 · HD269833 · HD269835 · HD269841 · HD269845 · HD269847 · HD269861 · HD269871 · HD269918 · HD37552 · NGC 2011 · NGC 2014 · NGC 2020 · NGC 2021 · And 5 more.

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Large Magellanic Cloud ; NGC 2030 et al

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Large Magellanic Cloud ; NGC 2030 et al

This image encompasses a fascinating complex of nebulae and stars, found north of the main bar of the Large Magellanic Cloud in the constellation Dorado. NGC 2029, NGC 2032 and NGC 2035 are star-forming regions, while NGC 2040 is a supernova remnant which contains an open cluster.
The blue "bubble" of NGC 2020 surrounds a Wolf-Rayet star and together with the adjacent red emission nebula NGC 2014 makes up what is called the Cosmic Reef.

Processed as an HOO image
Images taken from my back yard here in rural Western Australia Dec 23 - Jan 2024.

Original
B
Final
C

Objects of the South - negative declination only
Narrowband imaging
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The “AstroBin Image of the Day and Top Picks”, or IOTD/TP, is a long-running system to promote beautiful, interesting, peculiar, or otherwise amazing astrophotographs, with a focus on technical excellence. Learn more.

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Status	Advanced success
Started	...
Astrometry.net job	9122566
PixInsight job	X387486LZBPSWXAJK65FV5WC9GYNFCA4
PixInsight queue size	n/a
PixInsight stage	TASK_LOG

RA (center)	05h34m06s.376
RA (top/left)	05h33m52s.992
RA (top/right)	05h38m50s.936
RA (bottom/right)	05h34m19s.270
RA (bottom/left)	05h29m18s.758

Dec (center)	-67°35′10″.94
Dec (top/left)	-68°03′26″.81
Dec (top/right)	-67°27′21″.52
Dec (bottom/right)	-67°06′52″.55
Dec (bottom/left)	-67°42′28″.20

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Large Magellanic Cloud ; NGC 2030 et al

Large Magellanic Cloud ; NGC 2030 et al

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Image Index:

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Large Magellanic Cloud ; NGC 2030 et al

Large Magellanic Cloud ; NGC 2030 et al

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Description

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