Astronomy:NGC 4874

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NGC 4874
NGC 4874 dominates this picture created from optical and near-infrared exposures taken with the Wide Field Channel of Hubble's Advanced Camera for Surveys.
(Credit: ESA/Hubble, NASA)
Observation data (J2000 epoch)
ConstellationComa Berenices
Right ascension 12h 59m 35.709s[1]
Declination+27° 57′ 33.80″[1]
Redshift0.023907±0.00000667[2]
Helio radial velocity7,167±2 km/s[2]
Distance315.73 ± 6.41 Mly (96.804 ± 1.966 Mpc)[2]
Group or clusterComa Cluster
Apparent magnitude (V)11.4[3]
Apparent magnitude (B)13.7[4]
Characteristics
TypecD; Di
Size79.792 to 82.79 kpc (260,250 to 270,020 ly)
(diameter; D25.0 B-band and 2MASS K-band total isophotes[2]
Apparent size (V)1.9 × 1.9[2]
Other designations
UGC 8103, MCG+05-31-070, PGC 44628[2]

NGC 4874 is a supergiant elliptical galaxy in the constellation of Coma Berenices. It was discovered on 11 April 1785 by German-British astronomer William Herschel, who catalogued it as a bright patch of nebulous feature.[5] The second-brightest galaxy within the northern Coma Cluster, it is located at a distance of about 97 megaparsecs (316,000,000 light-years) from Earth.[6]

Characteristics

Template:Section unreferenced The galaxy is surrounded by an immense stellar halo that extends up to one million light-years in diameter.[7] It is also enveloped by a huge cloud of interstellar medium that is currently being heated by the action of infalling material from its central supermassive black hole. A jet of highly energetic plasma extends out to 1,700 light-years from its center. The galaxy has 18,700±2,260 globular clusters.

Supernovae

Three supernovae have been observed in NGC 4874:

  • SN 1968B (type unknown, mag. 17.4) was discovered by Fritz Zwicky on 3 February 1968.[8][9]
  • SN 1981G (Type Ia, mag. 15) was discovered by Miklós Lovas on 2 June 1981.[10][11]
  • SN 2025ilo (Type Ib, mag. 20.6) was discovered by A. Horti-David, K. Sarneczky, and J. Vinko on 26 April 2025.[12]

See also

References

  1. 1.0 1.1 "SIMBAD basic query result". SIMBAD Astronomical Database. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=NGC+4874&submit=SIMBAD+search. 
  2. 2.0 2.1 2.2 2.3 2.4 2.5 "NASA/IPAC Extragalactic Database". Results for NGC 4889. http://ned.ipac.caltech.edu/cgi-bin/objsearch?objname=NGC+4889&extend=no&hconst=67.80&omegam=0.268&omegav=0.683&corr_z=1&out_csys=Equatorial&out_equinox=J2000.0&obj_sort=RA+or+Longitude&of=pre_text&zv_breaker=30000.0&list_limit=5&img_stamp=YES. 
  3. Michard, R.; Andreon, S. (2008). "Morphology of galaxies in the Coma cluster region down to M_B = −14.25. I. A catalog of 473 members". Astronomy and Astrophysics 490 (3): 923. doi:10.1051/0004-6361:200810283. Bibcode2008A&A...490..923M. 
  4. Falco, Emilio E.; Kurtz, Michael J.; Geller, Margaret J.; Huchra, John P.; Peters, James; Berlind, Perry; Mink, Douglas J.; Tokarz, Susan P. et al. (1999). "The Updated Zwicky Catalog (UZC)". Publications of the Astronomical Society of the Pacific 111 (758): 438. doi:10.1086/316343. Bibcode1999PASP..111..438F. 
  5. Seligman, Courtney. "New General Catalogue Objects: NGC 4874". https://cseligman.com/text/atlas/ngc48a.htm#4874. 
  6. "Distance Results for NGC 4874". NASA. https://ned.ipac.caltech.edu/cgi-bin/nDistance?name=NGC+4874. 
  7. "Hubble Catches Galaxies Swarmed by Star Clusters - NASA Science" (in en-US). 2017-09-29. https://science.nasa.gov/missions/hubble/hubble-catches-galaxies-swarmed-by-star-clusters/. 
  8. Zwicky, F. (28 February 1968). Marsden, Brian G.. ed. "SUPERNOVA IN NGC 4874". Central Bureau for Astronomical Telegrams (IAU) 2056: 1. http://www.cbat.eps.harvard.edu/IAUCs/IAUC2056.jpg. Retrieved 2 December 2024. 
  9. "SN 1968B". IAU. https://www.wis-tns.org/object/1968B. 
  10. Szeidl, B.; Lovas, M.; Torres, C.; Gonzalez, E. (1981). "Supernovae". International Astronomical Union Circular (3610): 1. Bibcode1981IAUC.3610....1S. http://www.cbat.eps.harvard.edu/iauc/03600/03610.html#Item1. 
  11. "SN 1981G". IAU. https://www.wis-tns.org/object/1981G. 
  12. "SN 2025ilo". IAU. https://www.wis-tns.org/object/2025ilo.