Object type | H II region |
---|---|
Other designations | RCW 36, Gum 20, BBW 217[1][2] |
Constellation | Vela |
08h 59m 00.9s | |
Declination | −43° 44′ 10″ |
Distance | 2300 ly[3] / 700 pc |
In visual light (V) | |
15.2 | |
Size | 5 arcmin |
Estimated age | 1.1±0.6 Myr[4] |
Related media on Wikimedia Commons | |
RCW 36 (also designated Gum 20)[5] is an emission nebula containing an open cluster in the constellation Vela. This H II region is part of a larger-scale star-forming complex known as the Vela Molecular Ridge (VMR), a collection of molecular clouds in the Milky Way that contain multiple sites of ongoing star-formation activity.[1] The VMR is made up of several distinct clouds, and RCW 36 is embedded in the VMR Cloud C.
RCW 36 is one of the sites of massive-star formation closest to the Solar System,[6] whose distance of approximately 700 parsecs (2300 light-years). The most massive stars in the star cluster are two stars with late-O or early-B spectral types, but the cluster also contains hundreds of lower-mass stars.[4] This region is also home to objects with Herbig–Haro jets, HH 1042 and HH 1043.[7]