Astronomy:NGC 5936

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NGC 5936
NGC 5936 imaged by SDSS
Observation data (J2000 epoch)
ConstellationSerpens
Right ascension 15h 30m 00.8451s[1]
Declination+12° 59′ 21.472″[1]
Redshift0.013298[1]
Helio radial velocity3987 ± 3 km/s[1]
Distance198.7 ± 13.9 Mly (60.93 ± 4.27 Mpc)[1]
Apparent magnitude (V)12.5[1]
Characteristics
TypeSB(rs)b[1]
Size~81,400 ly (24.97 kpc) (estimated)[1]
Apparent size (V)1.4′ × 1.3′[1]
Other designations
IRAS 15276+1309, UGC 9867, MCG+02-39-030, PGC 55255[1]

NGC 5936 is a barred spiral galaxy in the constellation of Serpens. Its velocity with respect to the cosmic microwave background is 4131 ± 11 km/s, which corresponds to a Hubble distance of 60.93 ± 4.27 Mpc (~199 million light-years).[1] It was discovered by German-British astronomer William Herschel on 12 April 1784.[2]

NGC 5936 is listed as a luminous infrared galaxy (LIRG),[1] and as a field galaxy, i.e. one that does not belong to a larger galaxy group or cluster and hence is gravitationally alone.[3]

Supernovae

Two supernovae have been observed in NGC 5936:

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 1.11 "Results for object NGC 5936". NASA and Caltech. https://ned.ipac.caltech.edu/byname?objname=NGC+5936. 
  2. Seligman, Courtney. "New General Catalogue Objects: NGC 5936". https://cseligman.com/text/atlas/ngc59.htm#5936. 
  3. Turner, E. L.; Gott, J. R., III (1976). "Groups of galaxies. I. A catalog". The Astrophysical Journal Supplement Series 32: 409. doi:10.1086/190403. Bibcode1976ApJS...32..409T. 
  4. Kumar, S. (2013). "Supernova 2013dh in NGC 5936 = Psn J15300109+1259129". Central Bureau Electronic Telegrams (3561): 1. Bibcode2013CBET.3561....1K. 
  5. "SN 2013dh". IAU. https://www.wis-tns.org/object/2013dh. 
  6. "SN 2023awp". IAU. https://www.wis-tns.org/object/2023awp. 

Template:NGC objects:5500-5999