Hubbry Logo
NGC 4411BNGC 4411BMain
Open search
NGC 4411B
Community hub
NGC 4411B
logo
8 pages, 0 posts
0 subscribers
Be the first to start a discussion here.
Be the first to start a discussion here.
NGC 4411B
from Wikipedia

NGC 4411B
NGC 4411B imaged by the Vera C. Rubin Observatory
Observation data (J2000 epoch)
ConstellationVirgo
Right ascension12h 26m 47.2398s[1]
Declination+08° 53′ 04.619″[1]
Redshift0.004243±0.000003[1]
Heliocentric radial velocity1,272±1 km/s[1]
Distance73.06 ± 18.26 Mly (22.400 ± 5.600 Mpc)[1]
Group or clusterVirgo Cluster
Apparent magnitude (V)12.98[1]
Characteristics
TypeSAB(s)cd[1]
Size~68,000 ly (20.85 kpc) (estimated)[1]
Apparent size (V)2.5′ × 2.5′[1]
Other designations
KPG 336B, IRAS 12242+0909, UGC 7546, MCG +02-32-055, PGC 040745, CGCG 070-082[1]

NGC 4411B (also known as UGC 7546) is a barred spiral galaxy in the constellation of Virgo. Its velocity with respect to the cosmic microwave background is 1,610±24 km/s, which corresponds to a Hubble distance of 77.4 ± 5.5 Mly (23.74 ± 1.70 Mpc).[1] Two non-redshift measurements give a similar distance of 73.06 ± 18.26 Mly (22.400 ± 5.600 Mpc).[2] It was discovered by French astronomer Guillaume Bigourdan on 25 April 1895.[3] There was a longstanding confusion of identification between this galaxy and the neighboring spiral galaxy NGC 4411.[3] Therefore, this galaxy, despite its common name, was not a part of the original New General Catalogue.

NGC 4411B and NGC 4411 form a pair of galaxies, referred to as KPG 336.[4] Both galaxies are members of the Virgo Cluster.

NGC 4411B is a Seyfert II Galaxy, i.e. it has a quasar-like nucleus with very high surface brightnesses whose spectra reveal strong, high-ionisation emission lines, but unlike quasars, the host galaxy is clearly detectable.[5]

Supernovae

[edit]

Two supernovae have been observed in NGC 4411B.

See also

[edit]

References

[edit]
[edit]
Revisions and contributorsEdit on WikipediaRead on Wikipedia
Add your contribution
Related Hubs
User Avatar
No comments yet.