NGC 3811

Galaxy in the constellation Ursa Major From Wikipedia, the free encyclopedia

NGC 3811 is a barred spiral galaxy in the constellation of Ursa Major. Its velocity with respect to the cosmic microwave background is 3,299±15 km/s, which corresponds to a Hubble distance of 158.7 ± 11.1 Mly (48.65 ± 3.41 Mpc).[1] Additionally, 12 non-redshift measurements give a similar mean distance of 152.10 ± 12.53 Mly (46.633 ± 3.843 Mpc).[2] It was discovered by German-British astronomer William Herschel on 9 February 1788.[3]

Right ascension11h 41m 16.6161s[1]
Declination+47° 41 26.887[1]
Redshift0.010294±0.000009[1]
Quick facts Observation data (J2000 epoch), Constellation ...
NGC 3811
NGC 3811 imaged by SDSS
Observation data (J2000 epoch)
ConstellationUrsa Major
Right ascension11h 41m 16.6161s[1]
Declination+47° 41 26.887[1]
Redshift0.010294±0.000009[1]
Heliocentric radial velocity3,086±3 km/s[1]
Distance152.10 ± 12.53 Mly (46.633 ± 3.843 Mpc)[1]
Apparent magnitude (V)12.9[1]
Characteristics
TypeSB(r)cd[1]
Size~110,600 ly (33.91 kpc) (estimated)[1]
Apparent size (V)2.2′ × 1.7′[1]
Other designations
IRAS 11386+4758, UGC 6650, MCG +08-21-091, Mrk 185, PGC 36265, CGCG 242-074[1]
Close

NGC 3811 is a starburst galaxy.[1] It is also a galaxy whose nucleus shines in the ultraviolet range, and is thus listed in the Markarian catalogue as Mrk 185.[4]

Supernovae

Two supernovae have been observed in NGC 3811:

  • SN 1969C (type unknown, mag. 12) was discovered by Italian astronomer Leonida Rosino on 9 February 1969, and independently by Jankovits on 11 February 1969.[5][6]
  • SN 1971K (type unknown, mag. 16.1) was discovered by Russian amateur astronomer Piotr Grigor'evich Kulikovsky on 12 June 1971.[7][8]

See also

References

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