astro.wikisort.org - GalaxyNGC 5775 is a spiral galaxy, a member of the Virgo Cluster, that lies at a distance of about 70 million light-years. Although the spiral is tilted away from us, with only a thin sliver in view, such a perspective can be advantageous for astronomers. For instance, astronomers have previously used the high inclination of this spiral to study the properties of the halo of hot gas[4] that is visible when the galaxy is observed at X-ray wavelengths. It is a member of the NGC 5775 Group of galaxies, itself one of the Virgo III Groups strung out to the east of the Virgo Supercluster of galaxies.[5]
Spiral galaxy in the constellation Virgo
NGC 5775 |
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Constellation | Virgo |
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Right ascension | 14h 53m 57.653s[1] |
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Declination | +03° 32′ 40.10″[1] |
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Redshift | 0.005607[2] |
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Helio radial velocity | 1681[2] |
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Distance | 66.33 ± 13.31 Mly (20.338 ± 4.081 Mpc)[2] |
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Group or cluster | Virgo Cluster |
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Apparent magnitude (V) | 11.34 |
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Apparent magnitude (B) | 13.0 |
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Type | Sbc[3] |
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Apparent size (V) | 3.967' × 0.793'[1] |
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UGC 9579, MCG+01-38-014, PGC 53247[3] |
Interaction with NGC 5774
NGC 5775 is interacting with the nearby galaxy NGC 5774 in the form of two connecting H I bridges through which the gas is travelling from NGC 5774 to NGC 5775.[6]
Faint optical emission as well as radio continuum emission are also present along the bridges.[7]
It is possible that star formation is occurring between the galaxies.[6]
This system may be in the early stages of a merger.[7]
Gallery
References
- Skrutskie, Michael F.; Cutri, Roc M.; Stiening, Rae; Weinberg, Martin D.; Schneider, Stephen E.; Carpenter, John M.; Beichman, Charles A.; Capps, Richard W.; Chester, Thomas; Elias, Jonathan H.; Huchra, John P.; Liebert, James W.; Lonsdale, Carol J.; Monet, David G.; Price, Stephan; Seitzer, Patrick; Jarrett, Thomas H.; Kirkpatrick, J. Davy; Gizis, John E.; Howard, Elizabeth V.; Evans, Tracey E.; Fowler, John W.; Fullmer, Linda; Hurt, Robert L.; Light, Robert M.; Kopan, Eugene L.; Marsh, Kenneth A.; McCallon, Howard L.; Tam, Robert; Van Dyk, Schuyler D.; Wheelock, Sherry L. (1 February 2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131: 1163–1183. doi:10.1086/498708. ISSN 0004-6256.
- "NED results for object NGC 5775". National Aeronautics and Space Administration / Infrared Processing and Analysis Center. Retrieved 4 February 2017.
- "NGC 5775". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 4 February 2017.
- Li, Jiang-Tao; Li, Zhiyuan; Wang, Q. Daniel; Irwin, Judith A.; Rossa, Joern (October 2008). "Chandra Observation of the Edge-on Spiral NGC 5775: Probing the Hot Galactic Disk/Halo Connection". Monthly Notices of the Royal Astronomical Society. 390 (1): 59–70. arXiv:0807.3587. Bibcode:2008MNRAS.390...59L. doi:10.1111/j.1365-2966.2008.13749.x. S2CID 15029716.
- "The Virgo III Groups". Atlas of the Universe. Retrieved 2010-11-27.
- Irwin, Judith; Caron, Bryan (2003). "The NGC 5775/4 Interacting System". In Shlosman, Isaac (ed.). Mass-Transfer Induced Activity in Galaxies. Cambridge University Press. p. 362. ISBN 978-0-521-54330-9.
- Irwin, Judith A. (1994). "Arcs and bridges in the interacting galaxies NGC 5775/NGC 5774". The Astrophysical Journal. 429 (2): 618–633. Bibcode:1994ApJ...429..618I. doi:10.1086/174349.
External links
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NGC |
- NGC 5770
- NGC 5771
- NGC 5772
- NGC 5773
- NGC 5774
- NGC 5775
- NGC 5776
- NGC 5777
- NGC 5778
- NGC 5779
- NGC 5780
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Virgo constellation |
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Stars (list) | |
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Star clusters | |
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Nebulae | |
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Galaxies | Messier | |
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NGC | |
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Other |
- A1689-zD1
- Abell 1835 IR1916
- Arp 240 (NGC 5257 and NGC 5258)
- Arp 271 (NGC 5426 and NGC 5427)
- BR 1202-0725
- 3C 273
- 3C 279
- 3C 298
- 4C 04.42
- Eyes Galaxies
- GR 8
- IC 1011
- IC 1101
- IC 3258
- IC 3328
- IRAS 12212+0305
- IRAS 13197−1627
- M60-UCD1
- Markarian 50
- Markarian 1318
- PG 1216+069
- PG 1244+026
- PG 1254+047
- PG 1307+085
- PG 1416−129
- PG 1426+015
- PKS 1148-001
- PKS 1167+014
- PKS 1217+023
- PKS 1229−021
- PKS 1302−102
- PKS 1335−127
- PKS 1402+044
- PKS 1405−076
- QSO B1208+1011
- QSO B1243−072
- QSO B1246−057
- QSO B1331+170
- RXJ1242−11
- SMM J14011+0252
- UM 448
- UM 461
- UM 462
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Galaxy clusters | |
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Other |
- GRB 930131
- GRB 030328
- GRB 050408
- GRB 050801
- GRB 080310
- North Polar Spur
- SN 1960F
- SN 1981B
- SN 1990B
- SN 1990N
- SN 1991T
- SN 1991bg
- SN 1994D
- SN 1999br
- SN 2002cx
- SN 2007bi
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На других языках
[de] NGC 5775
NGC 5775 ist eine Balkenspiralgalaxie vom Hubble-Typ SBc und liegt im Sternbild Jungfrau am Nordsternhimmel. Sie gehört zum Virgo-Galaxienhaufen und ist rund 76 Millionen Lichtjahre von der Milchstraße entfernt. In optischer Nähe befinden sich die Galaxien NGC 5774 und IC 1070.
- [en] NGC 5775
[ru] NGC 5775
NGC 5775 (другие обозначения — UGC 9579, MCG 1-38-14, ZWG 48.60, KCPG 440B, IRAS14514+0344, PGC 53247) — спиральная галактика с перемычкой (SBc) в созвездии Дева.
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