astro.wikisort.org - Galaxy
NGC 1055 is an edge-on spiral galaxy located in the constellation Cetus. The galaxy has a prominent nuclear bulge crossed by a wide, knotty, dark lane of dust and gas. The spiral arm structure appears to be elevated above the galaxy's plane and obscures the upper half of the bulge. Discovered on December 19, 1783 by William Herschel from his home in Slough England.
| NGC 1055 | |
|---|---|
 Very Large Telescope image of NGC 1055 | |
| Observation data (J2000 epoch) | |
| Constellation | Cetus |
| Right ascension | 02h 41m 45.2s[1] |
| Declination | +00° 26′ 35″[1] |
| Redshift | 994 ± 5 km/s |
| Distance | 52 Mly (16 Mpc)[2] |
| Apparent magnitude (V) | 11.4[1] |
| Characteristics | |
| Type | SBb:[1] II-III: spindle[2] |
| Apparent size (V) | 7′.6 × 2′.7[1] |
| Other designations | |
| UGC 2173,[1] PGC 10208[1] | |
It is a binary system together with the bright spiral galaxy M77 (NGC 1068). These two are the largest galaxies of a small galaxy group that also includes NGC 1073, and five other small irregular galaxies.
NGC 1087, NGC 1090, and NGC 1094 appear close, but they simply appear in the field of view and are background galaxies.
Based on the published red shift, (Hubble Constant of 62 km/s per Mpc) a rough distance estimate for NGC 1055 is 52 million light-years, with a diameter of about 115,800 light-years. The separation between NGC 1055 and M77 is about 442,000 light-years.
NGC 1055 is a bright infrared and radio source, particularly in the wavelength for warm carbon monoxide. Astronomers believe that this results from unusually active star formation. It most likely has a transitional nucleus, however, there is a small chance that it could be a LINER.[3]
References
- NED (February 25, 2007), Results for search on NGC 1055
- Normandin, George (2002). "Edge-on Spiral Galaxy NGC 1055 in Cetus". Retrieved December 26, 2006
- Ho, Luis C.; Filippenko, Alexei V.; Sargent, Wallace L. W. (October 1997), "A Search for "Dwarf" Seyfert Nuclei. III. Spectroscopic Parameters and Properties of the Host Galaxies", Astrophysical Journal Supplement, vol. 112, no. 2, pp. 315–390, arXiv:astro-ph/9704107, Bibcode:1997ApJS..112..315H, doi:10.1086/313041, S2CID 17086638
External links
Media related to NGC 1055 at Wikimedia Commons- NGC 1055 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
- Edge-on Spiral Galaxy NGC 1055 in Cetus, Kopernik Observatory & Science Center, Vestal, New York
- Astronomy Picture of the Day - NGC 1055: Galaxy in a Box 24 April 2010
- ESO: A Galaxy on the Edge incl. Photos & Animations
На других языках
[de] NGC 1055
NGC 1055 ist eine Balken-Spiralgalaxie vom Hubble-Typ SBb im Sternbild Walfisch südlich der Ekliptik. Sie ist schätzungsweise 45 Mio. Lichtjahre von der Milchstraße entfernt und hat einen Durchmesser von etwa 100.000 Lj. Wahrscheinlich ist sie gravitativ an Messier 77 gebunden und gehört, wie auch NGC 1073, der M77-Galaxiengruppe an. Im selben Himmelsareal befinden sich weiterhin u. a. die Galaxien NGC 1032, NGC 1043, NGC 1068, NGC 1072.- [en] NGC 1055
[es] NGC 1055
NGC 1055 es una galaxia espiral barrada de tipo SBb que se encuentra en la constelación de Cetus a unos 52 millones de años luz de distancia. Su magnitud aparente es 11,4 y desde nuestra perspectiva prácticamente de lado.[ru] NGC 1055
NGC 1055 (другие обозначения — UGC 2173, MCG 0-7-81, ZWG 388.95, IRAS02391+0013, PGC 10208) — спиральная галактика с перемычкой (SBb) в созвездии Кит, находящаяся на расстоянии 55 млн световых лет от нас.Другой контент может иметь иную лицензию. Перед использованием материалов сайта WikiSort.org внимательно изучите правила лицензирования конкретных элементов наполнения сайта.
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