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NGC 918 is a barred spiral galaxy in the constellation Aries about 67 million light years from the Milky Way. It was discovered by John Herschel on Jan 11, 1831.[4]

NGC 918
NGC 918 by the Mount Lemmon SkyCenter
Observation data (J2000 epoch)
ConstellationAries
Right ascension02h 25m 50s[1]
Declination+18° 29′ 46″[1]
Redshift0.005027[2]
Helio radial velocity1507 ± 3 km/s[2]
Distance (comoving)20.6±1.5 mpc [3]
Apparent magnitude (V)15.01[1]
Apparent magnitude (B)16.0[1]
Characteristics
TypeSAB(rs)c[2]
Other designations
NGC 918,MCG+03-07-011, LEDA 9236[1]

The brightness class of NGC 918 is III and it has a broad line of neutral hydrogen. NGC 918 is also an active nucleus galaxy (AGN). Moreover, it is a field galaxy; that is to say, it does not belong to a cluster or group and is therefore gravitationally isolated.[5]

Many non-redshift measures give a distance of 19,115 ± 6,160 Mpc (~62,3 million ly),[6] which is within the distances calculated using the value shift.[3]

Two supernovae have been observed in this galaxy. SN 2009js was discovered in this galaxy October 11, 2009 at 17.2 magnitude.[5][7][8][9] This was the first subluminous supernova to be studied in infrared wavelengths.[10] Supernova SN 2011ek was discovered on Aug. 4, 2011 by Koichi Itagaki at 16.4 magnitude.[11][12]


References


  1. "NGC 918". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 19 June 2019.
  2. "NASA/IPAC Extragalactic Database". ned.ipac.caltech.edu. Retrieved 19 June 2019.
  3. We obtain the distance that separates us from a galaxy using Hubble's law: v = Hod, where Ho is the Hubble constant (70 ± 5 (km / s) / Mpc). The relative uncertainty Δd / d over the distance is equal to the sum of the relative uncertainties of the velocity and Ho.
  4. Seligman, Courtney. "New General Catalog Objects: NGC 900 - 949". New General Catalog Objects: NGC 900 - 949. Retrieved 19 June 2019.
  5. http://ned.ipac.caltech.edu/cgi-bin/nph-objsearch?objname=ngc+918&img_stamp=YES
  6. https://ned.ipac.caltech.edu/cgi-bin/nDistance?name=NGC+918
  7. "APOD: 2009 November 12 - Art and Science in NGC 918".
  8. SN 2009js at the Crossroads between Normal and Subluminous Type IIP Supernovae: Optical and Mid-infrared Evolution, The Astrophysical Journal, Volume 767, Issue 2, article id. 166, 15 pp. (2013).
  9. "Supernova 2009js in NGC 918".
  10. Gandhi, P.; Yamanaka, M.; Tanaka, M.; Nozawa, T.; Kawabata, K. S.; Saviane, I.; Maeda, K.; Moriya, T. J.; Hattori, T.; Sasada, M.; Itoh, R. (2013). "SN 2009js at the Crossroads between Normal and Subluminous Type IIP Supernovae: Optical and Mid-infrared Evolution". The Astrophysical Journal. 767 (2): 166. arXiv:1303.1565. Bibcode:2013ApJ...767..166G. doi:10.1088/0004-637X/767/2/166. S2CID 54036464.
  11. Nakano, S.; Yamaoka, H.; Kadota, K.; Tsuboi, M.; Balam, D. D.; Graham, M. L.; Hsiao, E. Y.; Green, D. W. E. (2011). "Supernova 2011ek near NGC 918 = PSN J02254889+1832000". Central Bureau Electronic Telegrams. 2783: 1. Bibcode:2011CBET.2783....1N.
  12. "Supernova 2011ek in NGC 918".



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[de] NGC 918

NGC 918 ist eine Balken-Spiralgalaxie vom Hubble-Typ SBc im Sternbild Widder auf der Ekliptik. Sie ist schätzungsweise 71 Millionen Lichtjahre von der Milchstraße entfernt und hat einen Durchmesser von etwa 70.000 Lj.
- [en] NGC 918

[ru] NGC 918

NGC 918 (другие обозначения — UGC 1888, MCG 3-7-11, ZWG 462.11, KARA 103, IRAS02230+1816, PGC 9236) — спиральная галактика с перемычкой (SBc) в созвездии Овен.


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