NGC 2805 explained

NGC 2805
Constellation Name:Ursa Major
Epoch:J2000
Type:SAB(rs)d[1]
Dist Ly:NaNMpc
Z:0.005779
H Radial V:1733 ± 1 km/s
Appmag V:11.0
Size V:6.3' x 4.8'
Size:~27.84kpc (estimated)

NGC 2805 is a intermediate spiral galaxy in the constellation of Ursa Major. Its velocity with respect to the cosmic microwave background is 1834 ± 7 km/s, which corresponds to a Hubble distance of 27.05 ± 1.90 Mpc (∼88.2 million light-years). However, 11 non redshift measurements give a distance of 12.76 ± 11.89 Mpc (41.6 million light-years).[2] (Note: this sample of measurements is inconsistent: seven values between 3.03 Mpc and 5.13 Mpc are reported in publications from 1984 to 1985, then four values between 26.8 Mpc and 28.8 Mpc.) The galaxy was discovered by German-British astronomer William Herschel on 2 April 1791.[3]

One supernova has been observed in NGC 2805: SN 2019hsw (type II, mag. 15.4).[4]

NGC 2805 Group

NGC 2805 is the namesake of the NGC 2805 group (also known as LGG 173), which includes at least 4 other galaxies: NGC 2814, NGC 2820, NGC 2880, and IC 2458.[5] This group, minus NGC 2880, are also collectively called Holmberg 124.[6]

See also

Notes and References

  1. Web site: NASA/IPAC Extragalactic Database . Results for NGC 2805 . 15 August 2024.
  2. Web site: Distance Results for NGC 2805 . NASA/IPAC EXTRAGALACTIC DATABASE . . 15 August 2024.
  3. Web site: NGC 2805 . Seligman . Courtney . Celestial Atlas . 15 August 2024 .
  4. Web site: Transient Name Server . SN 2019hsw . . 15 August 2024.
  5. 1993A&AS..100...47G . General study of group membership. II. Determination of nearby groups . Garcia . A. M. . Astronomy and Astrophysics Supplement Series . 1993 . 100 . 47 .
  6. 1937AnLun...6....1H . A Study of Double and Multiple Galaxies Together with Inquiries into some General Metagalactic Problems . Holmberg . Erik . Annals of the Observatory of Lund . 1937 . 6 . 1 .