02h 41m 45.2292s, +00° 26′ 35.988″NGC 1055
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| NGC 1055 | |
|---|---|
| Lua error in package.lua at line 80: module 'Module:InfoboxImage/data' not found. Very Large Telescope image of NGC 1055 | |
| Observation data (J2000 epoch) | |
| Constellation | Cetus |
| Right ascension | Template:RA[1] |
| Declination | Template:DEC[1] |
| Redshift | 0.003322±0.000002[1]Template:R/superscript |
| Heliocentric radial velocity | 996±1 km/s[1]Template:R/superscript |
| Distance | 52 Mly (16 Mpc)[2] |
| Apparent magnitude (V) | 11.4[1] |
| Characteristics | |
| Type | SBb:[1] II-III: spindle[2] |
| Size | ~114,400 ly (35.06 kpc) (estimated)[1]Template:R/superscript |
| Apparent size (V) | 7.6′ × 2.7′[1]Template:R/superscript |
| Other designations | |
| Template:Odlist[1] | |
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. It was discovered by German-British astronomer William Herschel on December 18, 1783, from his home in Slough, England.[3]
NGC 1055 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 redshift, (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 114,400 light-years. The separation between NGC 1055 and M77 is about 7 million 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.[4]
See also
References
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- ^ a b c d e f g h i Page Module:Citation/CS1/styles.css has no content."Results for object NGC 1055". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 30 May 2025.
- ^ a b Normandin, George (2002). "Edge-on Spiral Galaxy NGC 1055 in Cetus". Retrieved December 26, 2006
- ^ Page Module:Citation/CS1/styles.css has no content.Seligman, Courtney. "New General Catalogue Objects: NGC 1055 (=PGC 10208)". Celestial Atlas. Retrieved 30 May 2025.
- ^ Page Module:Citation/CS1/styles.css has no content.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
- Page Template:Sister-inline/styles.css has no content.Script error: No such module "Sister project logo". Media related to Script error: No such module "Commons link". at Wikimedia Commons
- Template:WikiSky
- 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
- SEDS – NGC 1055
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