Aja viide. Aja lugu.

NGC 1285 is a barred spiral galaxy in the constellation of Eridanus. Its velocity with respect to the cosmic microwave background is 5081 ± 12 km/s, which corresponds to a Hubble distance of 244.4 ± 17.1 Mly (74.94 ± 5.25 Mpc).^[1] However, three non-redshift measurements give a distance of 180.47 ± 3.24 Mly (55.333 ± 0.994 Mpc).^[2] It was discovered by Heinrich Louis d'Arrest on 28 October 1865.^[3]

Supernovae

Three supernovae have been observed in NGC 1285:

SN 2004F (type IIn-pec, mag. 17.8) was discovered by the Lick Observatory Supernova Survey on 16 January 2004.^[4]^[5]
SN 2013el (type Ib-pec, mag. 15.5) was discovered by Stu Parker on 11 July 2013.^[6]^[7]
SN 2017fvf (type IIP, mag. 17.81) was discovered by the Gaia Photometric Science Alerts programme on 30 July 2017.^[8]

^ ^a ^b ^c ^d ^e ^f ^g ^h ⁱ ^j ^k "Results for object NGC 1285". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 18 November 2024.
^ "Distance Results for NGC 1285". NASA/IPAC EXTRAGALACTIC DATABASE. NASA. Retrieved 18 November 2024.
^ Seligman, Courtney. "New General Catalogue Objects: NGC 1285". Celestial Atlas. Retrieved 18 November 2024.
^ Swift, B.; Burket, J.; Pugh, H.; Foley, R. J.; Filippenko, A. V.; Li, W.; Serduke, F. J. D.; Chornock, R. (2004). "Supernovae 2004D, 2004E, and 2004F". International Astronomical Union Circular (8271): 2. Bibcode:2004IAUC.8271....2S.
^ "SN 2004F". Transient Name Server. IAU. Retrieved 18 November 2024.
^ Parker, Stuart; Valenti, S.; Graham, M. L.; Howell, D. A.; Sand, D.; Parrent, J. T. (2013). "Supernova 2013el in NGC 1285 = PSN J03175245-0718021". Central Bureau Electronic Telegrams. 3611: 1. Bibcode:2013CBET.3611....1P.
^ "SN 2013el". Transient Name Server. IAU. Retrieved 18 November 2024.
^ "SN 2017fvf". Transient Name Server. IAU. Retrieved 18 November 2024.