Astronomy:NGC 3836

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NGC 3836
NGC 3836 imaged by SDSS
Observation data (J2000 epoch)
ConstellationCrater
Right ascension 11h 43m 29.7872s[1]
Declination−16° 47′ 45.244″[1]
Redshift0.012208±0.0000200[1]
Helio radial velocity3,660±6 km/s[1]
Distance193.5 ± 13.6 Mly (59.32 ± 4.17 Mpc)[1]
Apparent magnitude (V)13.5[1]
Characteristics
TypeSb pec[1]
Size~78,900 ly (24.19 kpc) (estimated)[1]
Apparent size (V)1.4′ × 1.3′[1]
Other designations
IRAS 11409-1631, MCG-03-30-010, PGC 36445[1]

NGC 3836 is a peculiar spiral galaxy in the constellation of Crater. Its velocity with respect to the cosmic microwave background is 4,022±26 km/s, which corresponds to a Hubble distance of 193.5 ± 13.6 Mly (59.32 ± 4.17 Mpc).[1] It was discovered by German astronomer Wilhelm Tempel on 29 April 1877.[2]

NGC 3836 is an active galaxy nucleus candidate, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars.[3]

Supernovae

Three supernovae have been observed in NGC 3836:

  • SN 2017rt (Type Ic, mag. 17.47) was discovered by Pan-STARRS on 10 January 2017.[4]
  • SN 2020aqe (Type II, mag. 18.269) was discovered by ATLAS on 23 January 2020.[5]
  • SN 2021aefs (Type IIn, mag. 18.36) was discovered by Gaia Photometric Science Alerts on 9 November 2021.[6]

See also

References

Coordinates: Sky map 11h 43m 29.7872s, −16° 47′ 45.244″