Astronomy:NGC 3389

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NGC 3389
NGC 3389 imaged by SDSS
Observation data (J2000 epoch)
ConstellationLeo
Right ascension 10h 48m 27.9204s[1]
Declination+12° 31′ 59.897″[1]
Redshift0.004346±0.000007[1]
Helio radial velocity1,303±2 km/s[1]
Distance71.70 ± 3.01 Mly (21.983 ± 0.924 Mpc)[1]
Group or clusterHOLM 212, NGC 3338 Group (LGG 214)
Apparent magnitude (V)12.3B[1]
Characteristics
TypeSA(s)c[1]
Size~81,000 ly (24.83 kpc) (estimated)[1]
Apparent size (V)2.8′ × 1.3′[1]
Other designations
HOLM 212C, NGC 3373, UGC 5914, MCG+02-28-013, PGC 32306[1]

NGC 3389 is a spiral galaxy in the constellation of Leo. Its velocity with respect to the cosmic microwave background is 1,651±24 km/s, which corresponds to a Hubble distance of 79.4 ± 5.7 Mly (24.35 ± 1.74 Mpc).[1] However, 24 non-redshift measurements give a closer mean distance of 71.70 ± 3.01 Mly (21.983 ± 0.924 Mpc).[2] It was discovered by German-British astronomer William Herschel on 11 March 1784.[3] It was also observed by John Herschel on 23 March 1830, causing it to be listed a second time in the New General Catalogue as NGC 3373.[3]

Holm 212 and NGC 3338 groups

NGC 3389, Messier 105, and NGC 3384 are listed together as Holm 212 in Erik Holmberg's A Study of Double and Multiple Galaxies Together with Inquiries into some General Metagalactic Problems, published in 1937.[4]

According to A. M. Garcia, NGC 3389 is a member of the NGC 3338 Group (also known as LGG 214). In addition to NGC 3338, this galaxy group includes at least three other galaxies: NGC 3346, UGC 5832, and MRK 1263.[5]

Supernovae

Two supernovae have been observed in NGC 3389.

See also

References

  1. ↑ 1.00 1.01 1.02 1.03 1.04 1.05 1.06 1.07 1.08 1.09 1.10 "Results for object NGC 3389". NASA and Caltech. https://ned.ipac.caltech.edu/byname?objname=NGC+3389. 
  2. ↑ "Distance Results for NGC 3389". NASA. https://ned.ipac.caltech.edu/cgi-bin/nDistance?name=NGC+3389. 
  3. ↑ 3.0 3.1 Seligman, Courtney. "New General Catalogue Objects: NGC 3389". https://cseligman.com/text/atlas/ngc33a.htm#3389. 
  4. ↑ Holmberg, Erik (1937). "A Study of Double and Multiple Galaxies Together with Inquiries into some General Metagalactic Problems". Annals of the Observatory of Lund 6: 1. Bibcode: 1937AnLun...6....1H. 
  5. ↑ Garcia, A. M. (1993). "General study of group membership. II. Determination of nearby groups". Astronomy and Astrophysics Supplement Series 100: 47. Bibcode: 1993A&AS..100...47G. 
  6. ↑ Martynov, D. Ya.; Haradze, E. K.; Chuadze, A. D. (1967). "Supernova in NGC 3389". International Astronomical Union Circular (2001): 1. Bibcode: 1967IAUC.2001....1M. http://www.cbat.eps.harvard.edu/iauc/02000/02001.html#Item1. 
  7. ↑ Bertola, F.; Detre, L.; Lovas, M. (1967). "Supernova in NGC 3389". International Astronomical Union Circular (2002): 1. Bibcode: 1967IAUC.2002....1B. http://www.cbat.eps.harvard.edu/iauc/02000/02002.html#Item1. 
  8. ↑ Bishop, David. "Other Supernovae Images". https://www.rochesterastronomy.org/snimages/snother.html#1967C. 
  9. ↑ "SN 1967C". IAU. https://www.wis-tns.org/object/1967C. 
  10. ↑ Borzov, G. G.; Dibai, É. A.; Esipov, V. F.; Pronik, V. I. (1 December 1969). "Observations of Chuadze's and Wild's Supernovae.". Soviet Astronomy 13: 423. ISSN 0038-5301. Bibcode: 1969SvA....13..423B. https://ui.adsabs.harvard.edu/abs/1969SvA....13..423B. 
  11. ↑ Nakano, S.; Yusa, T.; Kadota, K. (December 2009). "Supernova 2009md in NGC 3389". Central Bureau Electronic Telegrams 2065: 1. Bibcode: 2009CBET.2065....1N. http://www.cbat.eps.harvard.edu/cbet/002000/CBET002065.txt. 
  12. ↑ "SN 2009md". IAU. https://www.wis-tns.org/object/2009md. 

Coordinates: Sky map 10h 48m 27.9204s, +12° 31′ 59.897″



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