Astronomy:Cetus III

From HandWiki
Cetus lll
Observation data
ConstellationCetus
Right ascension 02h 05m 19.4s
Declination−04° 16′ 12.0″
Distance818,652 ly
Group or clusterMilky Way subgroup
Characteristics
TypeUltra-faint dwarf
Half-light radius (physical)90

Cetus lll is an ultra-faint dwarf galaxy (UFD) that is a satellite galaxy to the Milky Way. It is located at a distance of 251 kiloparsecs in the constellation of Cetus. It has a half-light radius of 90 parsecs.[1]

It was identified as a statistically significant overdensity of stars by the Subaru/Hyper Suprime-Cam Survey. Its small size made it invisible to the Sloan Digital Sky Survey.[1]

References

  1. 1.0 1.1 Homma, Daisuke; Chiba, Masashi; Okamoto, Sakurako; Komiyama, Yutaka; Tanaka, Masayuki; Tanaka, Mikito; Ishigaki, Miho N.; Hayashi, Kohei et al. (January 2018). "Searches for new Milky Way satellites from the first two years of data of the Subaru/Hyper Suprime-Cam survey: Discovery of Cetus III" (in en). Publications of the Astronomical Society of Japan 70: S18. doi:10.1093/pasj/psx050. ISSN 0004-6264. https://ui.adsabs.harvard.edu/abs/2018PASJ...70S..18H/abstract. 

NAME Cetus III Dwarf Galaxy on SIMBAD, Centre de données astronomiques de Strasbourg.