NGC 4244 explained
NGC 4244, also known as Caldwell 26, is an edge-on loose spiral galaxy in the constellation Canes Venatici, and is part of the M94 Group or Canes Venatici I Group, a galaxy group relatively close to the Local Group containing the Milky Way. In the sky, it is located near the yellow naked-eye star, Beta Canum Venaticorum, but also near the barred spiral galaxy NGC 4151 and irregular galaxy NGC 4214.
With an apparent V-band magnitude of 10.18,[1] NGC 4244 lies approximately 4.3 megaparsecs[1] (14 million light years)[6] away. A nuclear star cluster and halo is located near the centre of this galaxy.[6] [7]
See also
References
External links
Notes and References
- Web site: Results for object NGC 4244 (NGC 4244). NASA/IPAC Extragalactic Database. California Institute of Technology. 2021-02-09.
- 10.3847/1538-3881/153/1/6. The Local Tully–Fisher Relation for Dwarf Galaxies. 2016. Karachentsev. Igor D.. Kaisina. Elena I.. Kashibadze (Nasonova). Olga G.. The Astronomical Journal. 153. 6. 1611.02574. 119388974 . free .
- Web site: Search specification: NGC 4244. HyperLeda. Université Claude Bernard Lyon 1. 2021-02-09.
- The Night Sky Observers Guide, Vol. 2, pg 46. Kepple, G. and Sanner, G., Willmann-Bell Inc., 2002
- NGC 4244. 2021-02-09.
- Web site: A Rotating Compact Nuclear Stellar Cluster in NGC 4244. 31 July 2008. Gemini Observatory. 8 August 2008.
- CJO - Abstract - Detection of a stellar halo in NGC 4244 . Seth. A. . de Jong. R. . Dalcanton. J. . Proceedings of the International Astronomical Union . 2006. 2 . S241 . 523–524 . Cambridge University Press. 10.1017/S1743921307009003 . 119058120 . free .