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NGC 4618 information


NGC 4618
Barred spiral galaxy NGC 4618
Observation data (J2000 epoch)
ConstellationCanes Venatici[1]
Right ascension12h 41m 32.8s[2]
Declination+41° 09′ 03″[2]
Redshift544 ± 1 km/s[2]
Apparent magnitude (V)11.2[2]
Characteristics
TypeSB(rs)m[2]
Apparent size (V)4'.2 × 3'.4[2]
Notable featuresasymmetric; single spiral arm[3]
Other designations
IC 3667,[2] UGC 7853,[2] PGC 042575,[2] Arp 23,[2] VV 73[2]
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NGC 4618 is a distorted barred dwarf galaxy in the constellation Canes Venatici. The galaxy is formally classified as a Sm galaxy, which means that its structure vaguely resembles the structure of spiral galaxies. The galaxy is sometimes referred to as a Magellanic spiral because of its resemblance to the Magellanic clouds.

One supernova has been observed in NGC 4618: SN 1985F (type type Ib).[4]

  1. ^ R. W. Sinnott, ed. (1988). The Complete New General Catalogue and Index Catalogue of Nebulae and Star Clusters by J. L. E. Dreyer. Sky Publishing Corporation and Cambridge University Press. ISBN 978-0-933346-51-2.
  2. ^ a b c d e f g h i j k "NASA/IPAC Extragalactic Database". Results for NGC 4618. Retrieved 2006-11-15.
  3. ^ Cite error: The named reference carnegieatlas was invoked but never defined (see the help page).
  4. ^ Transient Name Server entry for SN 1985F. Retrieved 29 March 2023.

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