Astronomy:NGC 6744

From HandWiki
Short description: Galaxy in the constellation Pavo


NGC 6744
Wide Field Imager view of a Milky Way look-alike NGC 6744.jpg
Wide Field Imager view of a Milky Way look-alike NGC 6744
Observation data (J2000 epoch)
ConstellationPavo
Right ascension 19h 09m 46.1s[1]
Declination−63° 51′ 27″[1]
Redshift0.002805[1]
Helio radial velocity841 ± 2 km/s[1]
Distance31 ± 5.2 Mly
(9.5 ± 1.6 Mpc)[2]
Apparent magnitude (V)9.14[1]
Characteristics
TypeSAB(r)bc[1] II[citation needed]
Apparent size (V)20′.0 × 12′.9[1]
Other designations
Caldwell 101, PGC 62836

NGC 6744 (also known as Caldwell 101) 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.[3] It was discovered from Parramatta in Australia by Scottish astronomer James Dunlop on 30 June 1826.[4]

NGC 6744 lies within the Virgo Supercluster.[5][6]

One supernova has been observed in NGC 6744: SN 2005at (type Ic, mag. 16) was discovered on 15 March 2005.[7]

See also

References

External links