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NGC 7001

From Wikipedia, the free encyclopedia
Galaxy in the constellation Aquarius
NGC 7001
The intermediate spiral galaxy NGC 7001 (SDSS DR14)
Observation data (J2000epoch)
ConstellationAquarius
Right ascension21h 01m 07.7s[1]
Declination−00° 11′ 43″[1]
Redshift0.023714[1]
Heliocentric radial velocity7,109[1] km/s
Distance302 Mly (92.7 Mpc)[1]
Apparent magnitude (V)13.8[1]
Characteristics
TypeSAB(rs)ab[1]
Mass4.8×1011 (Stellar mass)[2] M
Size~123,100 ly (37.74 kpc) (estimated)[1]
Apparent size (V)1.25 × 1.06[1]
Other designations
NPM1G -00.0540,IRAS 20585-0023,UGC 11663,MCG +00-53-016,PGC 65905,CGCG 374-37[1]

NGC 7001 is anintermediate spiral galaxy[3] located about 300 millionlight-years away[3] in theconstellationAquarius.[4] NGC 7001 has an estimated diameter of 123,000 light-years.[3] It was discovered by English astronomerJohn Herschel on July 21, 1827, and was also observed by Austrian astronomer Rudolf Spitaler on September 26, 1891.[5]

NGC 7001 has tightly wound spiral arms similar to the galaxyNGC 488.[6] The galaxy is also host to asupermassive black hole with an estimated mass of 7 × 107M.[7]

See also

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References

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  1. ^abcdefghij"NASA/IPAC Extragalactic Database".Results for NGC 7001. Retrieved2017-04-13.
  2. ^Wilman, David J.; Fontanot, Fabio; De Lucia, Gabriella; Erwin, Peter; Monaco, Pierluigi (2013-08-01)."The hierarchical origins of observed galaxy morphology".Monthly Notices of the Royal Astronomical Society.433 (4):2986–3004.arXiv:1305.7163.Bibcode:2013MNRAS.433.2986W.doi:10.1093/mnras/stt941.ISSN 0035-8711.
  3. ^abc"Your NED Search Results".ned.ipac.caltech.edu. Retrieved2017-04-15.
  4. ^Rojas, Sebastián García."Galaxy NGC 7001 · Deep Sky Objects Browser".DSO Browser. Archived fromthe original on 2017-05-24. Retrieved2017-04-15.
  5. ^"New General Catalog Objects: NGC 7000 – 7049".cseligman.com. Retrieved2017-04-15.
  6. ^Buta, Ronald J. (2019-09-01)."The systematics of galaxy morphology in the comprehensive de Vaucouleurs revised Hubble-Sandage classification system: application to the EFIGI sample".Monthly Notices of the Royal Astronomical Society.488 (1):590–608.arXiv:1906.08124.Bibcode:2019MNRAS.488..590B.doi:10.1093/mnras/stz1693.ISSN 0035-8711.
  7. ^Arzoumanian, Zaven; Baker, Paul T.; Brazier, Adam; Brook, Paul R.; Burke-Spolaor, Sarah; Becsy, Bence; Charisi, Maria; Chatterjee, Shami; Cordes, James M.; Cornish, Neil J.; et al. (2021-06-01)."The NANOGrav 11 yr Data Set: Limits on Supermassive Black Hole Binaries in Galaxies within 500 Mpc".The Astrophysical Journal.914 (2): 121.arXiv:2101.02716.Bibcode:2021ApJ...914..121A.doi:10.3847/1538-4357/abfcd3.ISSN 0004-637X.

External links

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