2019年4月1日 · Sh2-232 (centre) and Sh2-235 (lower left) are large, faint regions of Ha-nebulosity in the constellation Auriga. But they aren’t the only objects in the image. The small oval structure just left of centre of Sh2-232 is a planetary nebula, PN G173.5+03.2. Another faint planetary appears as a small yellowish haze around a star just above Sh2-235.

Sh2-231, Sh2-232, Sh2-233 and Sh2-235 emission nebulae are located in the constellation Auriga at an approximate distance of 5,900 ly from the Earth. These objects are associated with a giant molecular cloud, G174+2.15, in the Perseus Arm of the Milky Way.

The large Sh2-232 and smaller but brighter Sh2-235 are predominantly Ha emission nebula regions in the constellations of Auriga at around 5900 light years distance. Sh2-235 also has a reasonably strong Oiii component, and a bit shows up in the band of Sh2-232.

SH2-235, as designated in the Sharpless catalog. It is a kidney shaped HII region formed when two large clouds of gas collided. The nebula is part of a larger complex consisting of SH 231,232 and 233. The complex lies in the constellation Auriga. The …

2019年7月11日 · Sh2-235 is an emission region in Auriga. I just stumbled across it in an Ha survey image, and noted that it seemed pretty bright for this area, so I put it on my list. Bright or not, it's rarely imaged on its own, but there are images with its much larger and fainter neighbors Sh2-231 and -232.

2015年12月21日 · SH2-235, as designated in the Sharpless catalog , is a kidney shaped HII region formed when two large clouds of gas collided. The nebula is part of a larger complex consisting of SH 231,232 and 233. The complex lies in the constellation Auriga . The distance to SH2-235 is somewhat unclear.

2017年3月12日 · Sh 2-231, 233, 235, 232は、ぎょしゃ座のIC 410から北東約4度ほどの位置にあり1つの大きな星間雲を形成していると考えられています。 距離はデータによれば約1800 pcとのことでIC 410を中心とする星間雲までの距離は3200 pcとされており距離データが正しければ2つ …

2018年1月5日 · They are from right to left, Sh2-232, the largest, Sh2-235, the brightest, Sh2-231, and 233, the smallest. These objects are all associated with a giant molecular cloud, G174+2.15, in the Perseus arm of the Milky Way. They are located in the direction of the Auriga constellation at an approximate distance of 5,900 light-years from the Earth.

2020年7月10日 · The H ii region Sh2-235 (S235 hereafter, Sharpless 1959) is the brightest H ii region among four close emission nebulae (the others being Sh2-231, Sh2-232, and Sh2-233) located in the giant molecular cloud G174+2.5 (Ladeyschikov et al. 2016) in the direction of the Aur OB1 association (Straižys, Drew & Laugalys 2010) in the Perseus Spiral Arm ...

Sh 2-235 is ionised by the O9.5 V star BD +35 1201. Avedisova places this nebula in star formation region SFR 173.61+2.80 with 54 components, including 7 masers, the smaller HI region BFS 46 and several Herbig-Haro objects.