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NGC 3008

From Wikipedia, the free encyclopedia
Galaxy in the constellation Ursa Major
NGC 3008
SDSS image of NGC 3008
Observation data (J2000 epoch)
Constellation Ursa Major
Right ascension 09h 49m 34.261s[1]
Declination +44° 06′ 09.71″[1]
Redshift 0.01595[1]
Heliocentric radial velocity 4783 km/s[1]
Distance 240.5 ± 16.9 Mly (73.73 ± 5.18 Mpc)[1]
Group or cluster NGC 2998 group
Apparent magnitude (B)15.23[2]
Characteristics
Type S0/a[1]
Other designations
MCG +07-20-059, PGC 28252[1]

NGC 3008 is a lenticular galaxy with an active galactic nucleus [3] in the constellation of Ursa Major,[4] discovered by William Parsons and his assistants.[5] It is about 40 thousand light years across, and with a recessional velocity of about 4,785 kilometers per second,[5] is at a distance of 240 million light-years from the Sun.[1]

It is a member of the NGC 2998 group, which also includes NGC 2998, NGC 3002, NGC 3005, NGC 3006, and a few others.[6] Among these galaxies, it has the lowest star formation rate, at 0.02 M per year.[7]

References

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  1. ^ a b c d e f g h "Results for object NGC 3008 (NGC 3008)". NASA/IPAC Extragalactic Database. California Institute of Technology. Retrieved 2021年02月14日.
  2. ^ "Search specification: NGC 3008". HyperLeda. Université Claude Bernard Lyon 1. Retrieved 2021年02月14日.
  3. ^ "NGC 3008 -- LINER-type Active Galaxy Nucleus". Simbad. Strasbourg astronomical Data Center. Retrieved 17 April 2020.
  4. ^ "NGC 3008". In-The-Sky.org. Retrieved 17 April 2020.
  5. ^ a b "Celestial Atlas". cseligman.com. Retrieved 17 April 2020.
  6. ^ "NAME NGC 2998 Group". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2021年02月14日.
  7. ^ Paudel, Sanjaya; Sengupta, Chandreyee; Yoon, Suk-Jin; Chhatkuli, Daya Nidhi (2020). "MCG+07-20-052: Interacting Dwarf Pair in a Group Environment". The Astronomical Journal. 159 (4): 141. arXiv:2002.10076 . Bibcode:2020AJ....159..141P. doi:10.3847/1538-3881/ab722f . S2CID 211258826.
[edit ]
  • Media related to NGC 3008 at Wikimedia Commons


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