Coordinates: Sky map 11h 49m 04.9143s, −09° 43′ 47.784″

NGC 3905

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NGC 3905
File:NGC 3905 PanS.jpg
NGC 3905 imaged by Pan-STARRS
Observation data (J2000 epoch)
ConstellationCrater
Right ascension11h 49m 04.9143s[1]
Declination−09° 43′ 47.784″[1]
Redshift0.019227±0.0000210[1]
Heliocentric radial velocity5,764±6 km/s[1]
Distance238.64 ± 20.80 Mly (73.167 ± 6.376 Mpc)[1]
Group or clusterLDC 824 group
Apparent magnitude (V)12.9B[1]
Characteristics
TypeSB(rs)c[1]
Size~155,400 ly (47.64 kpc) (estimated)[1]
Apparent size (V)1.9′ × 1.4′[1]
Other designations
IRAS 11465-0927, MCG -01-30-035, PGC 36909[1]

NGC 3905 is a barred spiral galaxy in the constellation of Crater. Its velocity with respect to the cosmic microwave background is 6,130±26 km/s, which corresponds to a Hubble distance of 294.9 ± 20.7 Mly (90.41 ± 6.34 Mpc).[1] However, six non-redshift measurements give a closer mean distance of 238.64 ± 20.80 Mly (73.167 ± 6.376 Mpc).[2] It was discovered by English astronomer Andrew Ainslie Common in 1880.[3]

NGC 3905 is 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.[4]

LDC 824 group

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NGC 3905 is a member of the LDC 824 group of galaxies. This group contains 18 galaxies, including NGC 3702, NGC 3721, NGC 3722, NGC 3723, NGC 3763, NGC 3771, NGC 3791, NGC 3854, NGC 3858, IC 2910, and seven others.[5][6]

Supernovae

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Three supernovae have been observed in NGC 3905:

See also

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References

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  • Error creating thumbnail: File missing Media related to Lua error in Module:Commons_link at line 62: attempt to index field 'wikibase' (a nil value). at Wikimedia Commons
  • NGC 3905 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images