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NGC 2708
The spiral galaxy NGC 2708.
Observation data (J2000 epoch)
ConstellationHydra
Right ascension08h 56m 08.05s[1]
Declination−03° 21′ 36.4″[1]
Redshift0.006698 [1]
Heliocentric radial velocity2008 ± 5 km/s[1]
Distance111.4 ± 7.9 Mly (34.15 ± 2.41 Mpc)[1]
Apparent magnitude (V)12.0[1]
Characteristics
TypeSAB(s)b pec?[1]
Size~98,800 ly (30.29 kpc) (estimated)[1]
Apparent size (V)2.7' x 1.4'[1]
Other designations
NGC 2727, PGC 25097, CGCG 005-034, MCG +00-23-015, IRAS 08535-0309, 2MASX J08560804-0321363[1]

NGC 2708 is a spiral galaxy in the constellation of Hydra. Its velocity with respect to the cosmic microwave background is 2315 ± 22 km/s, which corresponds to a Hubble distance of 34.15 ± 2.41 Mpc (∼111 million light-years).[1] It was discovered by German-British astronomer William Herschel on 6 January 1785.[2] This galaxy was also observed by British astronomer John Herschel on 12 March 1826, and later listed as NGC 2727.[2]

The SIMBAD database lists NGC 2708 as a Seyfert II galaxy,[3] i.e. a galaxy with a quasar-like nucleus with very high surface brightnesses whose spectra reveal strong, high-ionisation emission lines, but unlike quasars, the host galaxy is clearly detectable.

One supernova has been observed in NGC 2708: SN 2023bee (type Ia, mag. 17.3).[4]

NGC 2708 Group

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According to A.M. Garcia, NGC 2708 is part of the four member NGC 2708 group (also known as LGG 164). The other three galaxies are: NGC 2695, NGC 2699, and NGC 2706.[5]

See also

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References

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