astro.wikisort.org - GalaxyNGC 7090 is a spiral galaxy[8] in the southern constellation of Indus located about 31 million light-years away.[6] English astronomer John Herschel first observed this galaxy on 4 October 1834.[1][2]
Spiral galaxy in the constellation Indus
NGC 7090 |
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 NGC 7090 image from the Hubble Space Telescope combines orange light (colored blue here), infrared (colored red) and emissions from glowing hydrogen gas (also in red) [1][2] |
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Constellation | Indus |
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Right ascension | 21h 36m 28.865s[3] |
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Declination | −54° 33′ 26.35″[3] |
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Redshift | 0.002859±0.000020[4] |
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Helio radial velocity | 846 km/s[5] |
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Distance | 31.0 Mly (9.5 Mpc)[6] |
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Apparent magnitude (V) | 10.51[7] |
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Type | Scd[8] |
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Mass | Stellar: 5.47×109[6] M☉ |
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IRAS 21329-5446, 2MASX J21362886-5433263, NGC 7090, LEDA 67045[7] |
The morphological class of NGC 7090 is Scd,[8] indicating it is a spiral with loosely-wound and somewhat disorganized arms. The galactic plane is inclined at an angle of 89° to the line of sight from the Earth,[8] giving it an edge-on view. The combined mass of the stars in this galaxy is 5.5 billion times the mass of the Sun (M☉), while the star formation rate is ~0.5 M☉·yr−1.[6] As a result of star formation, the diffuse ionized gas in the galaxy has a complex organization, showing filaments, bubbles, and super-shells.[9]
Three transient ultraluminous X-ray sources have been detected in NGC 7090.[10][11]
Gallery
References
- "Hubble Sees NGC 7090 — An actively star-forming galaxy". Hubble Space Telescope. NASA. September 14, 2012. Retrieved 2022-01-09.
- "NGC 7090 — An actively star-forming galaxy". ESA/Hubble Picture of the Week. Retrieved 24 September 2012.
- Skrutskie, Michael F.; et al. (1 February 2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131: 1163–1183. Bibcode:2006AJ....131.1163S. doi:10.1086/498708. ISSN 0004-6256.
- de Vaucouleurs, G.; et al. (1991), Third reference catalogue of bright galaxies, 9, New York: Springer-Verlag
- Tully, R. Brent; et al. (August 3, 2016). "COSMICFLOWS-3". The Astronomical Journal. 152 (2): 50. arXiv:1605.01765. Bibcode:2016AJ....152...50T. doi:10.3847/0004-6256/152/2/50.
- Lianou, S.; et al. (November 2019). "Dust properties and star formation of approximately a thousand local galaxies". Astronomy & Astrophysics. 631: 19. arXiv:1906.02712. Bibcode:2019A&A...631A..38L. doi:10.1051/0004-6361/201834553. A38.
- "NGC 7090". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2022-01-09.
- Heesen, Volker; et al. (May 2016). "Advective and diffusive cosmic ray transport in galactic haloes". Monthly Notices of the Royal Astronomical Society. 458 (1): 332–353. arXiv:1602.04085. Bibcode:2016MNRAS.458..332H. doi:10.1093/mnras/stw360.
- Rossa, J.; et al. (September 2012). "The Morphological Diversity of DIG in Halos of Edge-on Spirals as Revealed by HST/ACS". In de Avillez, M.A. (ed.). The Role of the Disk-Halo Interaction in Galaxy Evolution: Outflow vs. Infall?. EAS Publication Series. Vol. 56. pp. 221–224. Bibcode:2012EAS....56..221R. doi:10.1051/eas/1256035.
- Liu, Zhu; et al. (July 2019). "X-ray properties of two transient ULX candidates in galaxy NGC 7090". Monthly Notices of the Royal Astronomical Society. 486 (4): 5709–5715. arXiv:1904.13044. Bibcode:2019MNRAS.486.5709L. doi:10.1093/mnras/stz1194.
- Walton, D. J.; et al. (February 2021). "A new transient ultraluminous X-ray source in NGC 7090". Monthly Notices of the Royal Astronomical Society. 501 (1): 1002–1012. arXiv:2011.08870. Bibcode:2021MNRAS.501.1002W. doi:10.1093/mnras/staa3666.
External links
Media related to NGC 7090 at Wikimedia Commons
Constellation of Indus |
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Stars | Bayer | |
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Variable | |
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HR |
- 7992
- 8027
- 8114
- 8152
- 8177
- 8211
- 8233
- 8249
- 8269
- 8271
- 8286
- 8303
- 8331
- 8352
- 8381
- 8527
- 8547
- 8672
- 8769
- 8794
- 8809
- 8855
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HD |
- 199642
- 200887
- 206429
- 208184
- 218497
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Other | |
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Galaxies | |
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 Category |
На других языках
[de] NGC 7090
NGC 7090 ist eine Balken-Spiralgalaxie vom Hubble-Typ SBc im Sternbild Indianer am Südsternhimmel. Sie ist schätzungsweise 36 Millionen Lichtjahre von der Milchstraße entfernt und hat einen Durchmesser von etwa 85.000 Lichtjahren.
- [en] NGC 7090
[ru] NGC 7090
NGC 7090 (другие обозначения — PGC 67045, ESO 188-12, AM 2133-544, IRAS21329-5446) — спиральная галактика с перемычкой (SBc) в созвездии Индеец.
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