NGC 5671
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| NGC 5671 | |
|---|---|
| File:NGC 5671 PanS.jpg NGC 5671 imaged by Pan-STARRS | |
| Observation data (J2000 epoch) | |
| Constellation | Ursa Minor |
| Right ascension | 14h 27m 42.0426s[1] |
| Declination | +69° 41′ 38.703″[1] |
| Redshift | 0.030074±0.000143[1] |
| Heliocentric radial velocity | 9,016±43 km/s[1] |
| Distance | 353.75 ± 10.07 Mly (108.460 ± 3.086 Mpc)[1] |
| Apparent magnitude (V) | 14.10[1] |
| Characteristics | |
| Type | SB(r)b[1] |
| Size | ~211,000 ly (64.68 kpc) (estimated)[1] |
| Apparent size (V) | 1.7′ × 1.2′[1] |
| Other designations | |
| IRAS F14269+6954, UGC 9297, MCG +12-14-006, PGC 51641, CGCG 337-014[1] | |
NGC 5671 is a large barred spiral galaxy in the constellation of Ursa Minor. Its velocity with respect to the cosmic microwave background is 9,058±43 km/s, which corresponds to a Hubble distance of 435.7 ± 30.6 Mly (133.59 ± 9.39 Mpc).[1] However, five non-redshift measurements give a closer mean distance of 353.75 ± 10.07 Mly (108.460 ± 3.086 Mpc).[2] It was discovered by German-British astronomer William Herschel on 6 May 1791.[3][4]
According to Abraham Mahtessian, NGC 5671 and UGC 9295 form a pair of galaxies.[5]
Supernovae
[edit | edit source]Two supernovae have been observed in NGC 5671:
- SN 2008be (Type IIn, mag. 18.5) was discovered by the Lick Observatory Supernova Search (LOSS) on 12 March 2008.[6][7]
- SN 2020dya (Type II, mag. 19.11) was discovered by the Zwicky Transient Facility on 4 March 2020.[8]
See also
[edit | edit source]References
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External links
[edit | edit source]- 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 5671 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
