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Emission Nebula - NGC 1491 (SH2-206)

NGC 1491 (also designated SH2-206 and LBN 704) is a bright emission nebula and HII region, located on the edge of a vast cloud region of neutral gas, about 10,700 light-years away in the Perseus arm of our Milky Way Galaxy in the constellation Perseus.

 

The blue 11.22 magnitude star (BD +50 ° 886) is illuminating the nebula while its strong stellar wind is “blowing” a bubble in the gas that immediately surrounds it. The intense radiation from the star is also eroding the gas clouds surrounding it. (Ref: annesastronomynews.com/photo-gallery-ii/nebulae-clouds/ng...)

 

Observation data: J2000 epoch

Subtype: H II region

Right ascension: 04h 03m 15.9s

Declination: +51° 18′ 54″

Distance: 9,800 ± 2,000 ly

Constellation: Perseus

 

Tech Specs: Sky-Watcher Esprit 120ED Telescope, ZWO AS2600mc-Pro running at 0C, Sky-Watcher EQ6R-Pro mount, Optolong L-eXtreme filter (2”), 37 x 300 second exposures, guided using a ZWO 30mm f/4 mini guide scope and ZWO 120 Mini, focus with a ZWO EAF, controlled with a ZWO ASIAir Pro. Processed using PixInsight and DSS. Image Date: September 1, 2022. Location: The Dark Side Observatory, Weatherly, PA, USA (Bortle Class 4).

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Uploaded on November 23, 2022