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NGC 4689

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NGC 4689
SDSS image of NGC 4689.
Observation data (J2000 epoch)
ConstellationComa Berenices
Right ascension12h 47m 45.5s[1]
Declination13° 45′ 46″[1]
Redshift0.005390/1616 km/s[1]
Distance54,025,244 ly[1]
Group or clusterVirgo Cluster
Apparent magnitude (V)11.6[1]
Characteristics
TypeSA(rs)bc, LINER[1]
Size~78,581.58 ly (estimated)[1]
Apparent size (V)4.3 x 3.5[1]
Other designations
PGC 43186, UGC 7965, VCC 2058[1]

NGC 4689 is a spiral galaxy located about 54 million light-years away[2] in the constellation of Coma Berenices.[3] NGC 4689 is also classified as a LINER galaxy.[2] NGC 4689 is inclined at an angle of about 36° which means that the galaxy is seen almost face-on to the Earth's line of sight.[4] NGC 4689 was discovered by astronomer William Herschel on April 12, 1784.[5] The galaxy is a member of the Virgo Cluster.[6][7]

Physical characteristics

NGC 4689 has ring-like feature in its inner regions. Surrounding the inner ring lies a zone of bright, flocculent spiral structure with a ring-like boundary. Outside this zone is a well-defined, diffuse outer ring which is an unusual feature for a late-type galaxy like NGC 4689.[7]

Star Formation

The star forming disk in NGC 4689 has been truncated which means that the amount of star formation has been reduced significantly. This truncation may have been caused by an interaction with intracluster medium of the Virgo Cluster causing the galaxy to lose much of its interstellar medium in an effect known as ram-pressure stripping.[7] Due to its reduced amount of star formation, NGC 4689 has been classified as an Anemic galaxy.[8]

  • A Smudged Fingerprint.[9]
    A Smudged Fingerprint.[9]


See also

References

  1. ^ a b c d e f g h i "NASA/IPAC Extragalactic Database". Results for NGC 4689. Retrieved 2017-09-25.
  2. ^ a b "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2017-09-29.
  3. ^ Rojas, Sebastián García. "Galaxy NGC 4689 - Barred Spiral Galaxy in Coma Berenices Constellation · Deep Sky Objects Browser". DSO Browser. Retrieved 2017-09-29.
  4. ^ Kuno, Nario; Sato, Naoko; Nakanishi, Hiroyuki; Hirota, Akihiko; Tosaki, Tomoka; Shioya, Yasuhiro; Sorai, Kazuo; Nakai, Naomasa; Nishiyama, Kota; Vila-Vilaro ́, Baltsar (2007). "Nobeyama CO Atlas of Nearby Spiral Galaxies: Distribution of Molecular Gas in Barred and Non-barred Spiral Galaxies". Publications of the Astronomical Society of Japan. 59: 117–166. arXiv:0705.2678. Bibcode:2007PASJ...59..117K. doi:10.1093/pasj/59.1.117. S2CID 14076941.
  5. ^ "New General Catalog Objects: NGC 4650 - 4699". cseligman.com. Retrieved 2017-09-29.
  6. ^ "The Virgo Cluster". www.atlasoftheuniverse.com. Retrieved 2017-09-30.
  7. ^ a b c "NGC 4689 - (R)SA(rs)bc". The de Vaucouleurs Atlas of Galaxies. Retrieved 2017-09-28.
  8. ^ Elmegreen, Debra Meloy; Elmegreen, Bruce G.; Frogel, Jay A.; Eskridge, Paul B.; Pogge, Richard W.; Gallagher, Andrew; Iams, Joel (2 May 2002). "Arm Structure in Anemic Spiral Galaxies". The Astronomical Journal. 124 (2): 777–781. arXiv:astro-ph/0205105. Bibcode:2002AJ....124..777E. doi:10.1086/341613. S2CID 7757634.
  9. ^ "A Smudged Fingerprint". Retrieved 17 February 2020.
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