| NGC 6261 | |
|---|---|
| NGC 6261 imaged by Sloan Digital Sky Survey | |
| Observation data (J2000 epoch) | |
| Constellation | Hercules |
| Right ascension | 16h 56m 30.526s [1] |
| Declination | +27° 58′ 39.24″ [1] |
| Redshift | 0.035184 |
| Heliocentric radial velocity | 10,601 km/s |
| Distance | 471.4 Mly (144.53 Mpc) |
| Apparent magnitude (V) | 14.5 |
| Surface brightness | 28.5 mag/arcsec |
| Characteristics | |
| Type | S0/a |
| Size | 200,000 ly |
| Other designations | |
| PGC 59286, UGC 10617, MCG +05-40-006, CGCG 169-013, 2MASX J16563054+2758392, SDSS J165630.51+275839.0, UZC J165630.6+275839, NSA 070084, NVSS J165630+275838, LEDA 59286 | |
NGC 6261 is a lenticular galaxy in the constellation of Hercules. [2] [3] It is located 470 million light-years away from the Solar System and has an approximate diameter of 200,000 light-years. [4]
NGC 6261 was discovered on July 13, 1880, by French astronomer Edouard Stephan. [5] The galaxy is described as LINER according to SIMBAD database [1] and presents emission spectrum in its nucleus which is categorized by broad lines of weak ionized atoms.
Two supernovae have been discovered in NGC 6261: SN 2007hu and SN 2008dt.
SN 2007hu [6] was discovered on September 9, 2007, by astronomers Ernesto Guido, A. Sehgal and Tim Puckett. [7] It had a magnitude of 17.7 and was located 1".3 west and 1".4 north of the nucleus. The supernova was Type la. [6]
SN 2008dt [8] was discovered on 30 June, 2008, [9] by astronomers D. Madison, W. Li and A.V. Filippenko at the University of California, Berkeley. [10] It had a magnitude of 17.2 and was located 1".0 east and 5.5" south of the nucleus. [11] The supernova was Type la. [8]