Best H Ii

NGC 6188 is an emission nebula located within the Ara constellation. It’s recognized for its intricate dust structures, sculpted by ultraviolet light emanating from the nearby NGC 6193 star cluster. This nebula actively forms stars and is of interest to amateur astronomers and researchers studying s...

NGC 3576 is an emission nebula located within the Carina Nebula cluster. It’s notable for its prominent, pillar-like structures of dust and gas, illuminated by intense ultraviolet radiation from young, hot stars. These formations are actively involved in star formation. Astronomers and researchers s...

NGC 2174 is an emission nebula within the Orion constellation. It’s notable for its distinctive resemblance to a primate's head, created by dense clouds of hydrogen gas ionized by young, hot stars. This region is actively forming new stars and is primarily observed by astronomers studying star forma...

Messier 43 is an emission nebula located within the Orion constellation. It’s notable for being a relatively isolated star-forming region, distinct from the larger Orion Nebula. The nebula contains abundant hydrogen-II gas, indicating active star formation. Astronomers and amateur observers study it...

Sharpless 2-157 is an emission nebula located within the Cassiopeia constellation. Identified by astronomer Stewart Sharpless as part of his 1959 survey of star-forming regions, it’s notable for its strong hydrogen-alpha (HII) emission lines. These lines reveal intense star formation activity within...

The Ghost Head Nebula, designated NGC 2080, is an emission nebula in the Large Magellanic Cloud known for its two distinct bright spots that resemble glowing ghostly eyes.

The Running Chicken Nebula, also known as IC 2944, is an open cluster with nebulosity in Centaurus that is famous for housing Bok globules first discovered there in 1955.

NGC 2014 is a massive emission nebula located in the Large Magellanic Cloud, notable for its reddish glow and its close association with the neighboring blue nebula NGC 2020.

Sharpless 2-112 is an HII emission nebula included in American astronomer Stewart Sharpless's influential 1959 catalog of galactic nebulae.

Sharpless 2-235 is a massive star-forming region and emission nebula documented by Stewart Sharpless in his landmark 1959 catalog of HII regions.

IC 2948, the Lambda Centauri Nebula, is an emission cloud in Centaurus notable for containing dense, collapsing Bok globules observed by A.D. Thackeray.

NGC 371 is an open star cluster surrounded by an emission nebula in the Small Magellanic Cloud, known for its high concentration of massive, variable supergiant stars.

NGC 2467, the Skull and Crossbones Nebula, is an active star-forming region in the constellation Puppis, first discovered by William Herschel in 1784.

Sharpless 2-297 is a striking red emission nebula in the constellation Canis Major, famously cataloged by Stewart Sharpless in his 1959 survey.

NGC 2467, nicknamed the Skull and Crossbones, is an active star-forming region in the constellation Puppis, distinguished by its dark dust lanes that resemble a glowing human skull.

NGC 248 is an emission nebula located in the Small Magellanic Cloud, a dwarf satellite galaxy of the Milky Way that was observed and cataloged by James Dunlop in 1826.

Sharpless 2-263 is a diffuse emission nebula included in the 1959 Sharpless catalog, which mapped hundreds of HII regions across the Milky Way.

Sharpless 2-1 is an emission nebula cataloged by American astronomer Stewart Sharpless in his 1959 HII region survey of the Milky Way galaxy.

NGC 1714 is an emission nebula located within the Large Magellanic Cloud, a satellite galaxy of the Milky Way that was first observed by astronomer James Dunlop in 1826.

The Bubble Nebula in Barnard's Galaxy is a massive H II region located within the irregular dwarf galaxy NGC 6822, which was discovered by E. E. Barnard in 1884.

N41 is an emission nebula located in the Large Magellanic Cloud, originally cataloged by American astronomer Karl Henize in his 1956 survey.

DWB 20 is a faint emission nebula in the Cygnus X complex, cataloged by astronomers Dickel, Wendker, and Bieritz during their 1969 radio survey.

NGC 1715 is an emission nebula in the Large Magellanic Cloud that is notable for its distinct, bubble-like appearance, historically categorized by John Herschel in 1834.

NGC 249 is a diffuse emission nebula situated within the Small Magellanic Cloud, notable for being studied extensively by the Hubble Space Telescope to map cosmic dust.

DWB 169 is a galactic emission nebula in the Cygnus X star-forming region, identified in the 1969 DWB radio continuum survey of the Milky Way.

DWB 175 is a notable HII region within the Cygnus X complex, first cataloged by Dickel, Wendker, and Bieritz in their comprehensive 1969 survey.

NGC 256 is an open star cluster located in the Small Magellanic Cloud within the constellation Tucana, which was first cataloged by British astronomer John Herschel in 1834.

NGC 261 is an extensive emission nebula located in the Small Magellanic Cloud, a dwarf galaxy roughly 200,000 light-years away from Earth in the constellation Tucana.

Designated Sh2-264, the Lambda Orionis Nebula is a faint emission cloud in Orion, distinguished by its vast ring of glowing hydrogen gas surrounding the multiple star system Meissa.