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NGC 828

Coordinates:Sky map02h 10m 09.5476s, +39° 11′ 24.925″
From Wikipedia, the free encyclopedia
Galaxy in the constellation Andromeda

NGC 828
NGC 828 imaged byPan-STARRS
Observation data (J2000epoch)
ConstellationAndromeda
Right ascension02h 10m 09.5476s[1]
Declination+39° 11′ 24.925″[1]
Redshift0.017846[1]
Heliocentric radial velocity5350 ± 4 km/s[1]
Distance246.2 ± 17.3 Mly (75.49 ± 5.29 Mpc)[1]
Apparent magnitude (V)12.3[1]
Characteristics
TypeSa? pec[1]
Size~227,600 ly (69.77 kpc) (estimated)[1]
Apparent size (V)2.5′ × 1.6′[1]
Other designations
IRAS 02071+3857,2MASX J02100957+3911253,UGC 1655,MCG +06-05-092,PGC 8283,CGCG 522-125[1]

NGC 828 is aspiral galaxy in theconstellation ofAndromeda. Its velocity with respect to thecosmic microwave background is 5200 ± 17 km/s, which corresponds to aHubble distance of 250.2 ± 17.5 Mly (76.70 ± 5.37 Mpc).[1] Additionally, threenon-redshift measurements give a closer distance of 223.52 ± 7.06 Mly (68.533 ± 2.165 Mpc).[2] It was discovered by German-British astronomerWilliam Herschel on 18 October 1786.[3]

NGC 828 is aLINER galaxy, i.e. it has a type of nucleus that is defined by its spectral line emission which has weakly ionized or neutral atoms, while the spectral line emission from strongly ionized atoms is relatively weak.[1] In addition, NGC 828 is classified as aradio galaxy.[4]

Onesupernova has been observed in NGC 828:SN 2024lea (Type Ib, mag. 19.1) was discovered by theZwicky Transient Facility on 10 June 2024.[5]

See also

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References

[edit]
  1. ^abcdefghijkl"Results for object NGC 0828".NASA/IPAC Extragalactic Database.NASA andCaltech. Retrieved31 July 2024.
  2. ^"Distance Results for NGC 828".NASA/IPAC EXTRAGALACTIC DATABASE.NASA. Retrieved14 December 2024.
  3. ^Seligman, Courtney."New General Catalogue Objects: NGC 828".Celestial Atlas. Retrieved14 December 2024.
  4. ^"NGC 828".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved14 December 2024.
  5. ^"SN 2024lea".Transient Name Server.IAU. Retrieved14 December 2024.

External links

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