NGC 35 is a spiral galaxy in the constellation Cetus. It was discovered on November 21, 1886 by the astronomer Lewis A. Swift.[4]

NGC 35
NGC 35 PanS.jpg
Pan-STARRS image of NGC 35
Observation data (J2000 epoch)
ConstellationCetus
Right ascension00h 11m 10.49324s[1]
Declination−12° 01′ 14.6953″[1]
Redshift0.020096[2]
Helio radial velocity5964 km/s[2]
Distance273.8 Mly (83.95 Mpc)[3]
Characteristics
TypeSb[3]
Other designations
MCG-02-01-033, PGC 784[2]

ReferencesEdit

  1. ^ a b Brown, 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. ^ a b c "NGC 35". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-02-07.
  3. ^ a b Iglesias‐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: 38–51. doi:10.1086/502628. S2CID 17135800.
  4. ^ Seligman, Courtney. "New General Catalogue objects: NGC 1 - 49". cseligman.com. Retrieved 2021-02-07.

External linksEdit