NGC 2565

Galaxy in the constellation Cancer From Wikipedia, the free encyclopedia

NGC 2565 is a barred spiral galaxy in the constellation of Cancer. Its velocity with respect to the cosmic microwave background for is 3,814±16 km/s, which corresponds to a Hubble distance of 183.5 ± 12.9 Mly (56.26 ± 3.95 Mpc).[1] Additionally, 34 non-redshift measurements give a distance of 169.79 ± 4.64 Mly (52.057 ± 1.422 Mpc).[2] It was discovered by German-British astronomer J. Gerhard Lohse (bio-fr) in 1886.[3]

Right ascension08h 19m 48.3092s[1]
Declination+22° 01 53.087[1]
Redshift0.011948[1]
Quick facts Observation data (J2000 epoch), Constellation ...
NGC 2565
NGC 2565 imaged by SDSS
Observation data (J2000 epoch)
ConstellationCancer
Right ascension08h 19m 48.3092s[1]
Declination+22° 01 53.087[1]
Redshift0.011948[1]
Heliocentric radial velocity3,582±1 km/s[1]
Distance183.5 ± 12.9 Mly (56.26 ± 3.95 Mpc)[1]
Group or clusterNGC 2545 group (LGG 156)
Apparent magnitude (V)12.6[1]
Characteristics
Type(R')SBbc?[1]
Size~106,600 ly (32.68 kpc) (estimated)[1]
Apparent size (V)1.9′ × 0.9′[1]
Other designations
IRAS 08168+2211, UGC 4334, MCG +04-20-026, Mrk 386, PGC 23362, CGCG 119-057[1]
Close

NGC 2565 is a galaxy whose nucleus shines brightly in the ultraviolet. It is listed in the Markarian catalogue as Mrk 386.[4]

NGC 2565 is surrounded by a ring, and is a starburst galaxy, as indicated by its entry in the NASA/IPAC Extragalactic Database.[1]

NGC 2545 Group

NGC 2565 is a member of the NGC 2545 group (also known as LGG 156). The other galaxies in the group are NGC 2545 [fr], UGC 4308 [d], CGCG 119-044 [d], and CGCG 119-56.[5][6]

Supernovae

Two supernovae have been observed in NGC 2565:

  • SN 1960M (Type I, mag. 17) was discovered by Brazilian astronomer Alércio Moreira Gomes [pt] on 26 October 1960.[7][8]
  • SN 1992I (Type II, mag. 18) was discovered by French amateur astronomer Christian Buil [fr] on 29 February 1992.[9][10]

See also

References

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