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NGC 3389
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| NGC 3389 | |
|---|---|
 NGC 3389 imaged by SDSS | |
| Observation data (J2000 epoch) | |
| Constellation | Leo |
| Right ascension | 10h 48m 27.9204s[1] |
| Declination | +12° 31′ 59.897″[1] |
| Redshift | 0.004346±0.000007[1] |
| Heliocentric radial velocity | 1,303±2 km/s[1] |
| Distance | 71.70 ± 3.01 Mly (21.983 ± 0.924 Mpc)[1] |
| Group or cluster | HOLM 212, NGC 3338 Group (LGG 214) |
| Apparent magnitude (V) | 12.3B[1] |
| Characteristics | |
| Type | SA(s)c[1] |
| Size | ~81,000 ly (24.83 kpc) (estimated)[1] |
| Apparent size (V) | 2.8′ × 1.3′[1] |
| Other designations | |
| HOLM 212C, NGC 3373, UGC 5914, MCG +02-28-013, PGC 32306, CGCG 066-022[1] | |
NGC 3389 is a spiral galaxy in the constellation of Leo. Its velocity with respect to the cosmic microwave background is 1,651±24 km/s, which corresponds to a Hubble distance of 79.4 ± 5.7 Mly (24.35 ± 1.74 Mpc).[1] However, 24 non-redshift measurements give a closer mean distance of 71.70 ± 3.01 Mly (21.983 ± 0.924 Mpc).[2] It was discovered by German-British astronomer William Herschel on 11 March 1784.[3] It was also observed by John Herschel on 23 March 1830, causing it to be listed a second time in the New General Catalogue as NGC 3373.[3]
Holm 212 and NGC 3338 groups
[edit]NGC 3389, Messier 105, and NGC 3384 are listed together as Holm 212 in Erik Holmberg's A Study of Double and Multiple Galaxies Together with Inquiries into some General Metagalactic Problems, published in 1937.[4]
According to A. M. Garcia, NGC 3389 is a member of the NGC 3338 Group (also known as LGG 214). In addition to NGC 3338, this galaxy group includes at least three other galaxies: NGC 3346, UGC 5832, and MRK 1263.[5]
Supernovae
[edit]Two supernovae have been observed in NGC 3389.
See also
[edit]References
[edit]- ^ a b c d e f g h i j k "Results for object NGC 3389". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 23 July 2025.
- ^ "Distance Results for NGC 3389". NASA/IPAC EXTRAGALACTIC DATABASE. NASA. Retrieved 23 July 2025.
- ^ a b Seligman, Courtney. "New General Catalogue Objects: NGC 3389". Celestial Atlas. Retrieved 23 July 2025.
- ^ Holmberg, Erik (1937). "A Study of Double and Multiple Galaxies Together with Inquiries into some General Metagalactic Problems". Annals of the Observatory of Lund. 6: 1. Bibcode:1937AnLun...6....1H.
- ^ Garcia, A. M. (1993). "General study of group membership. II. Determination of nearby groups". Astronomy and Astrophysics Supplement Series. 100: 47. Bibcode:1993A&AS..100...47G.
- ^ Martynov, D. Ya.; Haradze, E. K.; Chuadze, A. D. (1967). "Supernova in NGC 3389". International Astronomical Union Circular (2001): 1. Bibcode:1967IAUC.2001....1M.
- ^ Bertola, F.; Detre, L.; Lovas, M. (1967). "Supernova in NGC 3389". International Astronomical Union Circular (2002): 1. Bibcode:1967IAUC.2002....1B.
- ^ Bishop, David. "Other Supernovae Images". Rochester Astronomy. Retrieved 23 July 2025.
- ^ "SN 1967C". Transient Name Server. IAU. Retrieved 23 July 2025.
- ^ Borzov, G. G.; Dibai, É. A.; Esipov, V. F.; Pronik, V. I. (1 December 1969). "Observations of Chuadze's and Wild's Supernovae". Soviet Astronomy. 13: 423. Bibcode:1969SvA....13..423B. ISSN 0038-5301.
- ^ Nakano, S.; Yusa, T.; Kadota, K. (December 2009). "Supernova 2009md in NGC 3389". Central Bureau Electronic Telegrams. 2065: 1. Bibcode:2009CBET.2065....1N.
- ^ "SN 2009md". Transient Name Server. IAU. Retrieved 23 July 2025.
External links
[edit]
Media related to NGC 3389 at Wikimedia Commons- NGC 3389 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
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