Galaxy in the constellation Coma Berenices
| NGC 4571 |
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| Observation data (J2000 epoch) |
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| Constellation | Coma Berenices |
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| Right ascension | 12h 36m 56.4s[1] |
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| Declination | +14° 13′ 02″[1] |
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| Redshift | 342 ± 3 km/s[1] |
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| Distance | 58 ± 11 Mly (17.7 ± 3.4 Mpc) |
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| Apparent magnitude (V) | 11.8[1] |
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| Characteristics |
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| Type | SA(r)d[1] |
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| Apparent size (V) | 3.6′ × 3.2′[1] |
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| Other designations |
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| NGC 4571, IC 3588[1] UGC 7788,[1] PGC 42100, VCC 1696[1] |
NGC 4571 is a spiral galaxy located in the constellation of Coma Berenices that William Herschel thought was Messier 91 in Charles Messier' catalog of deep-sky objects,[2] before nearly two centuries later that object was determined to be the nearby barred spiral galaxy NGC 4548.
Physical properties
The finding of Cepheids by the Canada France Hawaii Telescope in 1994 has established that this galaxy is a member of the Virgo Cluster.[2]
Despite being classified as a late-type galaxy, NGC 4571 has features more typical of spiral galaxies of earlier Hubble type such as a high color index, both low star formation rate and H-Alpha brightness, and relatively little neutral hydrogen,[3] suggesting it may have lost most of its gas due to interactions with Virgo's intragalactic medium and/or past interactions with other galaxies of the cluster.[4][5][6]
The low-surface brightness galaxy Malin 1 is located close to this object.[7] It is totally unrelated, however as it lies at a much higher distance.
Gallery
References
- ^ a b c d e f g h i "NASA/IPAC Extragalactic Database". Results for NGC 4571. Retrieved 2013-05-18.
- ^ a b Students for the Exploration and Development of Space NGC 4571, Accessed online 14 April 2011
- ^ Kennicutt, R. C. Jr. (1983). "On the evolution of the spiral galaxies in the Virgo cluster". The Astronomical Journal. 88: 483–488. Bibcode:1983AJ.....88..483K. doi:10.1086/113334.
- ^ Kennicutt, R. C. Jr. (1985). "An H I and optical study of the gas poor Virgo cluster spiral NGC 4571". ESO Workshop on the Virgo Cluster of Galaxies, Garching, West Germany, September 4–7, 1984. 88: 91–94. Bibcode:1985ESOC...20...91K. doi:10.1086/113334.
- ^ Kenney, J. D.; Young, J. S. (1986). "CO in H I-deficient Virgo cluster spiral galaxies". The Astrophysical Journal Letters. 301: L13–L17. Bibcode:1986ApJ...301L..13K. doi:10.1086/184614.
- ^ van der Hulst, J. M.; Skillman, E. D.; Kennicutt, R. C.; Bothun, G. D. (1987). "The neutral hydrogen content of red spiral galaxies". Astronomy and Astrophysics. 177: 63–70. Bibcode:1987A&A...177...63V.
- ^ Bothun, Gregory D.; Impey, Christopher D.; Malin, David F.; Mould, Jeremy R. (1987). "Discovery of a huge low-surface-brightness galaxy - A protodisk galaxy at low redshift?". The Astronomical Journal. 94: 23–29. Bibcode:1987AJ.....94...23B. doi:10.1086/114443.
External links
Media related to NGC 4571 at Wikimedia Commons- SEDS – NGC 4571
| NGC | |
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| PGC | - PGC 42096
- PGC 42097
- PGC 42098
- PGC 42099
- PGC 42100
- PGC 42101
- PGC 42102
- PGC 42103
- PGC 42104
|
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| UGC | - UGC 7784
- UGC 7785
- UGC 7786
- UGC 7787
- UGC 7788
- UGC 7789
- UGC 7790
- UGC 7791
- UGC 7792
|
|---|
NGC 4571 by Hubble Space Telescope
NGC 4571 (SDSS DR14)
Category
