Cannabaceae

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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One thought on “Cannabaceae

  1. Well, that’s interesting to know that Psilotum nudum are known as whisk ferns. Psilotum nudum is the commoner species of the two. While the P. flaccidum is a rare species and is found in the tropical islands. Both the species are usually epiphytic in habit and grow upon tree ferns. These species may also be terrestrial and grow in humus or in the crevices of the rocks.
    View the detailed Guide of Psilotum nudum: Detailed Study Of Psilotum Nudum (Whisk Fern), Classification, Anatomy, Reproduction

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