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NGC 3884
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| NGC 3884 | |
|---|---|
 SDSS image of NGC 3884 | |
| Observation data (J2000 epoch) | |
| Constellation | Leo |
| Right ascension | 11h 46m 12.1878s[1] |
| Declination | +20° 23′ 30.023″[1] |
| Redshift | 0.023123[1] |
| Heliocentric radial velocity | 6932 ± 2 km/s[1] |
| Distance | 334.80 ± 31.76 Mly (102.650 ± 9.738 Mpc)[1] |
| Group or cluster | Leo Cluster |
| Apparent magnitude (V) | 13.5[1] |
| Characteristics | |
| Type | SA(r)0/a, LINER[1] |
| Size | ~243,500 ly (74.65 kpc) (estimated)[1] |
| Apparent size (V) | 1.64′ × 1.10′[1] |
| Other designations | |
| UGC 6746, MCG +04-28-051, PGC 36706, CGCG 127-052[1] | |
NGC 3884 is a spiral galaxy located about 330 million light-years away[2] in the constellation Leo.[3] The galaxy was discovered by astronomer William Herschel on April 27, 1785[4] and is a member of the Leo Cluster.[5][6][7]
Although it is classified as a LINER galaxy,[8][9] NGC 3884 is also classified as a type 1 Seyfert galaxy.[2][10]
One supernova has been observed in NGC 3884. SN 2018yn (type Ic, mag. 18) was discovered by POSS on February 23, 2018.[11][12]
See also
[edit]References
[edit]- ^ a b c d e f g h i j "Results for object NGC 3884". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 2018-08-08.
- ^ a b "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-08-09.
- ^ "Revised NGC Data for NGC 3884". spider.seds.org. Retrieved 2018-08-09.
- ^ "New General Catalog Objects: NGC 3850 - 3899". cseligman.com. Retrieved 2018-07-17.
- ^ J., Donas; V., Buat; B., Milliard; M., Laget (August 1990). "Ultraviolet observations of galaxies in nearby clusters. I - Star formation rate in spiral galaxies of Abell 1367". Astronomy and Astrophysics. 235: 60. Bibcode:1990A&A...235...60D. ISSN 0004-6361.
- ^ "NGC 3884". Retrieved 2018-08-09.
- ^ "Hierarchy catalogue". leda.univ-lyon1.fr. Retrieved 2018-08-09.
- ^ "NGC 3884". Retrieved 2018-08-09.
- ^ "Detailed Object Classifications". ned.ipac.caltech.edu. Retrieved 2018-08-09.
- ^ Reddy, Naveen A.; Yun, Min S. (2004). "Radio and Far-Infrared Emission as Tracers of Star Formation and Active Galactic Nuclei in Nearby Cluster Galaxies". The Astrophysical Journal. 600 (2): 695–715. arXiv:astro-ph/0309649. Bibcode:2004ApJ...600..695R. doi:10.1086/379871. ISSN 0004-637X. S2CID 15068448.
- ^ "SN 2018yn". Transient Name Server. IAU. Retrieved 8 May 2025.
- ^ Bishop, David. "Bright Supernovae - 2018". rochesterastronomy.org. Retrieved 2018-08-09.
External links
[edit]
Media related to NGC 3884 at Wikimedia Commons- NGC 3884 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
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