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NGC 35

From Wikipedia, the free encyclopedia
Spiral galaxy in the constellation Cetus
NGC 35
Pan-STARRS image of NGC 35
Observation data (J2000epoch)
ConstellationCetus
Right ascension00h 11m 10.49324s[1]
Declination−12° 01′ 14.6953″[1]
Redshift0.020096[2]
Heliocentric radial velocity5964 km/s[2]
Distance273.8 Mly (83.95 Mpc)[3]
Characteristics
TypeSb[3]
Other designations
MCG -02-01-033,PGC 784[2]

NGC 35 is aspiral galaxy in the constellationCetus. It was discovered on November 21, 1886 by the astronomerLewis A. Swift.[4]

See also

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References

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  1. ^abBrown, A. G. A.; et al. (Gaia collaboration) (August 2018)."Gaia Data Release 2: Summary of the contents and survey properties".Astronomy & Astrophysics.616. A1.arXiv:1804.09365.Bibcode:2018A&A...616A...1G.doi:10.1051/0004-6361/201833051.
  2. ^abc"NGC 35".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2021-02-07.
  3. ^abIglesias‐Paramo, J.; Buat, V.; Takeuchi, T. T.; Xu, K.; Boissier, S.; Boselli, A.; Burgarella, D.; Madore, B. F.; Gil De Paz, A.; Bianchi, L.; Barlow, T. A.; Byun, Y.‐I.; Donas, J.; Forster, K.; Friedman, P. G.; Heckman, T. M.; Jelinski, P. N.; Lee, Y.‐W.; Malina, R. F.; Martin, D. C.; Milliard, B.; Morrissey, P. F.; Neff, S. G.; Rich, R. M.; Schiminovich, D.; Seibert, M.; Siegmund, O. H. W.; Small, T.; Szalay, A. S.; et al. (2006). "Star Formation in the Nearby Universe: The Ultraviolet and Infrared Points of View".The Astrophysical Journal Supplement Series.164 (1):38–51.arXiv:astro-ph/0601235.Bibcode:2006ApJS..164...38I.doi:10.1086/502628.S2CID 17135800.
  4. ^Seligman, Courtney."New General Catalogue objects: NGC 1 - 49".cseligman.com. Retrieved2021-02-07.

External links

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