Jump to content

NGC 5784

Coordinates: Sky map 14h 54m 16.4726s, +42° 33′ 28.356″
From Wikipedia, the free encyclopedia

NGC 5784
The lenticular galaxy NGC 5784
Observation data (J2000 epoch)
ConstellationBoötes
Right ascension14h 54m 16.4726s[1]
Declination+42° 33′ 28.356″[1]
Redshift0.017912[1]
Heliocentric radial velocity5370 ± 16 km/s[1]
Distance264.2 ± 18.5 Mly (81.01 ± 5.68 Mpc)[1]
Apparent magnitude (V)12.4[1]
Characteristics
TypeS0[1]
Size~149,400 ly (45.82 kpc) (estimated)[1]
Apparent size (V)1.9′ × 1.8′[1]
Other designations
IRAS 14524+4245, 2MASX J14541645+4233279, UGC 9592, MCG +07-31-006, PGC 53265, CGCG 221-009[1]

NGC 5784 is a lenticular galaxy in the constellation of Boötes. Its velocity with respect to the cosmic microwave background is 5493 ± 18 km/s, which corresponds to a Hubble distance of 81.01 ± 5.68 Mpc (∼264 million light-years).[1] It was discovered by German-British astronomer William Herschel on 9 April 1787.[2]

Supernovae

[edit]

Two supernovae have been observed in NGC 5784:

NGC 5739 Group

[edit]

According to Abraham Mahtessian, NGC 5784 is part of the seven member NGC 5739 group (also known as [M98j] 234). The other six galaxies are: NGC 5598, NGC 5603, NGC 5696, NGC 5739, NGC 5787, and NGC 5860.[5]

See also

[edit]

References

[edit]
  1. ^ a b c d e f g h i j k "Results for object NGC 5784". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 8 August 2024.
  2. ^ Seligman, Courtney. "New General Catalogue Objects: NGC 5784". Celestial Atlas. Retrieved 16 December 2024.
  3. ^ "SN 2018mef". Transient Name Server. IAU. Retrieved 16 December 2024.
  4. ^ "SN 2023bch". Transient Name Server. IAU. Retrieved 16 December 2024.
  5. ^ Mahtessian, A. P. (1998). "Groups of galaxies. III. Some empirical characteristics". Astrophysics. 41 (3): 308–321. doi:10.1007/BF03036100.
[edit]