NGC 6744 explained
NGC 6744 |
Epoch: | J2000 |
Type: | SAB(r)bc[1] II |
Z: | 0.002805 |
Dist Ly: | 31 ± 5.2 Mly [2] |
Appmag V: | 9.14 |
Size V: | 20′.0 × 12′.9 |
Constellation Name: | Pavo |
Names: | Caldwell 101, PGC 62836 |
NGC 6744 (also known as Caldwell 101 or the Pavo Galaxy[3]) is an intermediate spiral galaxy about 30 million light-years away[2] in the constellation Pavo (Peacock). It is considered as a Milky Way mimic in the immediate vicinity, displaying flocculent (fluffy) arms and an elongated core. It also has at least one distorted companion galaxy (NGC 6744A) superficially similar to one of the Magellanic Clouds.[4] It was discovered from Parramatta in Australia by Scottish astronomer James Dunlop on 30 June 1826.[5]
NGC 6744 lies within the Virgo Supercluster.[6] [7]
One supernova has been observed in NGC 6744: SN 2005at (type Ic, mag. 16) was discovered on 15 March 2005.[8]
See also
External links
Notes and References
- Web site: NASA/IPAC Extragalactic Database . Results for NGC 6744 . 2006-08-31 .
- Web site: Distance Results for NGC 6744 . NASA/IPAC Extragalactic Database . 2010-06-19.
- Book: Stoyan, Ronald. Schurig. Stephan. interstellarum Deep Sky Atlas. Cambridge University Press; Oculum-Verlag GmbH. Erlangen. 2014. 978-1-107-50338-0. 920437579.
- Web site: NASA/IPAC Extragalactic Database . Results for NGC 6744A . 2010-06-19.
- Web site: NGC Objects: NGC 6700–6749. 14 February 2019. cseligman.com. Seligman, Courtney.
- P. Fouque . E. Gourgoulhon . P. Chamaraux . G. Paturel. Groups of galaxies within 80 Mpc. II – The catalogue of groups and group members . Astronomy and Astrophysics Supplement . 1992 . 93 . 211–233 . 1992A&AS...93..211F.
- Web site: Nearby Groups of Galaxies. ned.ipac.caltech.edu. 2018-05-04.
- https://www.wis-tns.org/object/2005at Transient Name Server entry for SN 2005at.