NGC 524
NGC 524 is a lenticular galaxy in the constellation Pisces. It is at a distance of about 90 million light-years away from Earth. In the central bulge of the galaxy is visible gas forming a spiral structure.[2] It is the largest galaxy in a small galaxy group, the NGC 524 group, which is associated with NGC 488 and its group.[3] It was discovered by William Herschel in 1786. Two supernovae have been observed in the galaxy, SN 2000cx, a type Ia-p peaking at 14.5 magnitude, and SN 2008Q, type Ia.[4]
NGC 524 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Pisces |
Right ascension | 01h 24m 47.7s[1] |
Declination | +09° 32′ 20″[1] |
Redshift | 2403 ± 5 km/s[1] |
Distance | 86.1 ± 13.7 Mly (26.4 ± 4.2 Mpc)[1] |
Apparent magnitude (V) | 10.5 |
Characteristics | |
Type | SA(rs)0+[1] |
Apparent size (V) | 2′.8 × 2′.8[1] |
Other designations | |
UGC 968, PGC 5222[1] |
Gallery
- The lenticular galaxy NGC 524 as imaged by SDSS.
References
- "NASA/IPAC Extragalactic Database". Results for NGC 524. Retrieved 2006-11-18.
- Hubble Eyes a Mysterious Old Spiral
- Dmitry Makarov and Igor Karachentsev (2011). "Galaxy groups and clouds in the local (z∼ 0.01) Universe". MNRAS. 412 (4): 2498–2520. arXiv:1011.6277. Bibcode:2011MNRAS.412.2498M. doi:10.1111/j.1365-2966.2010.18071.x. S2CID 119194025. Retrieved 1 January 2016.
- List of Supernovae IAU Central Bureau for Astronomical Telegrams. Retrieved 29 December 2015.
External links
- Media related to NGC 524 at Wikimedia Commons
- NGC 524 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
- SEDS
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