NGC 4088

NGC 4088 is an intermediate spiral galaxy in the constellation Ursa Major. The galaxy forms a physical pair with NGC 4085, which is located 11′ away.[4]

NGC 4088
NGC 4088
NGC 4088 2MASS (near-infrared)
Observation data (J2000 epoch)
ConstellationUrsa Major[1]
Right ascension12h 05m 34.2s[2]
Declination+50° 32′ 21″[2]
Redshift0.002524[2]
Heliocentric radial velocity757 ± 1 km/s[2]
Distance51.5 ± 4.5 Mly
(15.8 ± 1.4 Mpc)[3]
Apparent magnitude (V)11.2[2]
Characteristics
TypeSAB(rs)bc[2]
Apparent size (V)5.8′ × 2.2′[2]
Other designations
UGC 7081,[2] PGC 38302,[2] Arp 18,[2] VV 357[2]

General information
Amateur image of NGC 4088, left, and companion NGC 4085, right.

NGC 4088 is a grand design spiral galaxy.[5] This means that the spiral arms in the galaxy's disk are sharply defined. In visible light, one of the spiral arms appears to have a disconnected segment. Halton Arp included this galaxy in the Atlas of Peculiar Galaxies as one of several examples where this phenomenon occurs.[6]

NGC 4088 and NGC 4085 are members of the M109 Group, a group of galaxies located in the constellation Ursa Major. This large group contains between 41 and 58 galaxies, including the spiral galaxy M109.[7][8][9]


Supernovae

Three supernovae have been observed in NGC 4088. The first was discovered on 10 February 1991, SN 1991G (Type II, mag. 17).[10]

On April 13, 2009, supernova SN 2009dd was discovered in NGC 4088.[11] At apparent magnitude 13.8,[11] it became the third-brightest supernova of 2009.[12]

On 16 May 2022, SN 2022jzc was discovered (Type II, mag. 17.8).[13]

References
  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. "NASA/IPAC Extragalactic Database". Results for NGC 4088. Retrieved 2006-11-16.
  3. "Distance Results for NGC 4088". NASA/IPAC Extragalactic Database. Retrieved 2010-05-17.
  4. A. Sandage; J. Bedke (1994). Carnegie Atlas of Galaxies. Washington, D.C.: Carnegie Institution of Washington. ISBN 978-0-87279-667-6.
  5. D. M. Elmegreen; B. G. Elmegreen (1987). "Arm classifications for spiral galaxies". Astrophysical Journal. 314: 3–9. Bibcode:1987ApJ...314....3E. doi:10.1086/165034.
  6. H. Arp (1966). "Atlas of Peculiar Galaxies". Astrophysical Journal Supplement. 14: 1–20. Bibcode:1966ApJS...14....1A. doi:10.1086/190147.
  7. R. B. Tully (1988). Nearby Galaxies Catalog. Cambridge: Cambridge University Press. ISBN 978-0-521-35299-4.
  8. A. Garcia (1993). "General study of group membership. II - Determination of nearby groups". Astronomy and Astrophysics Supplement. 100: 47–90. Bibcode:1993A&AS..100...47G.
  9. G. Giuricin; C. Marinoni; L. Ceriani; A. Pisani (2000). "Nearby Optical Galaxies: Selection of the Sample and Identification of Groups". Astrophysical Journal. 543 (1): 178–194. arXiv:astro-ph/0001140. Bibcode:2000ApJ...543..178G. doi:10.1086/317070. S2CID 9618325.
  10. Transient Name Server entry for SN 1991G. Retrieved 21 March 2023.
  11. "Supernova 2009dd in NGC 4088". Astronomy Section, Rochester Academy of Science. 2009-12-30. Retrieved 2010-05-17.
  12. David Bishop. "Bright Supernovae - 2009". supernovae.net (International Supernovae Network). Archived from the original on 2011-09-27. Retrieved 2010-06-04.
  13. Transient Name Server entry for SN 2022jzc. Retrieved 21 March 2023.
Wikimedia Commons has media related to NGC 4088.
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.