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). It was discovered by German astronomer Wilhelm Tempel on 29 April 1877. 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.
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. SN 2020aqe (Type II, mag. 18.269) was discovered by ATLAS on 23 January 2020. SN 2021aefs (Type IIn, mag. 18.36) was discovered by Gaia Photometric Science Alerts on 9 November 2021.
See also List of NGC objects (3001–4000)
References
External links Media related to NGC 3836 at Wikimedia Commons NGC 3836 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


