Galaxy in the constellation Canes Venatici)
| NGC 4774 |
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 The ring galaxy NGC 4774. |
| Observation data (J2000 epoch) |
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| Constellation | Canes Venatici |
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| Right ascension | 12h 53m 06.2s[1] |
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| Declination | +36° 49′ 22″[1] |
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| Redshift | 0.027823[1] |
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| Heliocentric radial velocity | 8341 ± 17 km/s[1] |
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| Distance | 412.8 ± 28.9 Mly (126.56 ± 8.87 Mpc)[1] |
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| Apparent magnitude (V) | 14.3[1] |
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| Characteristics |
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| Type | RING?[1] |
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| Size | ~74,800 ly (22.93 kpc) (estimated)[1] |
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| Apparent size (V) | 0.6' x 0.4'[1] |
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| Other designations |
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| IRAS 12507+3705, MCG +06-28-037, PGC 43759, CGCG 188-026, VV 789[1] |
NGC 4774, also known as the Kidney Bean Galaxy,[2] is a ring galaxy in the constellation of Canes Venatici. Its velocity with respect to the cosmic microwave background is 8581 ± 24 km/s, which corresponds to a Hubble distance of 126.56 ± 8.87 Mpc (∼413 million light-years).[1] It was discovered by German-British astronomer William Herschel on 17 March 1787.[2]
Two supernovae have been observed in NGC 4774: SN 2013he (type II-P, mag. 16.5),[3] and SN 2021cjd (type II-P, mag. 20.2).[4]
See also
- List of NGC objects (4001–5000)
References
- ^ a b c d e f g h i j k "NASA/IPAC Extragalactic Database". Results for NGC 4774. Retrieved 29 July 2024.
- ^ a b Celestial Atlas entry for NGC 4744. Retrieved 29 July 2024.
- ^ Transient Name Server entry for SN 2013he. Retrieved 29 July 2024.
- ^ Transient Name Server entry for SN 2021cjd. Retrieved 29 July 2024.
External links
Media related to NGC 4774 at Wikimedia Commons- NGC 4774 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
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