NGC 1288
Composite image of NGC 1288 taken with the Very Large Telescope. Supernova SN 2006dr is visible just to the left of the nucleus. | |
Observation data | |
---|---|
Constellation | Fornax |
Right ascension | 03h 17m 13.176s[1] |
Declination | –32° 34′ 33.08″[1] |
Redshift | 0.01500[2] |
Helio radial velocity | 4,497[2] km/s |
Distance | 196 Mly (60 Mpc)[3] |
Type | SABc(rs)[4] |
Mass/Light ratio | 14[3] M☉/L☉ |
Apparent dimensions (V) | 2′.2 × 1′.8[5] |
NGC 1288 is a barred spiral galaxy located about 196[3] million light years away in the constellation Fornax.[5] In the nineteenth century, English astronomer John Herschel described it as "very faint, large, round, very gradually little brighter middle." The morphological classification of SABc(rs)[4] indicates weak bar structure across the nucleus (SAB), an incomplete inner ring orbiting outside the bar (rs), and the multiple spiral arms are moderately wound (c).[6] The spiral arms branch at intervals of 120° at a radius of 30″ from the nucleus. The galaxy is most likely surrounded by a dark matter halo, giving it a mass-to-light ratio of 14 M☉/L☉.[3]
On July 17, 2006, a supernova with a magnitude of 16.1 was imaged in this galaxy from Pretoria, South Africa, at 12″ east and 2″ of the galactic core.[7] Designated SN 2006dr, it was determined to be a type Ia supernova.[8]
References
- ↑ 1.0 1.1 Skrutskie, M. F. et al. (February 2006), "The Two Micron All Sky Survey (2MASS)", Astrophysical Journal 131 (2): 1163–1183, Bibcode:2006AJ....131.1163S, doi:10.1086/498708.
- ↑ 2.0 2.1 Jones, D. Heath et al. (October 2009), "The 6dF Galaxy Survey: final redshift release (DR3) and southern large-scale structures", Monthly Notices of the Royal Astronomical Society 399 (2): 683–698, arXiv:0903.5451, Bibcode:2009MNRAS.399..683J, doi:10.1111/j.1365-2966.2009.15338.x.
- ↑ 3.0 3.1 3.2 3.3 Fuchs, B. et al. (December 1999), "Quantitative interpretation of the morphology of NGC 1288", Astronomy and Astrophysics 352: L36–L39, Bibcode:1999A&A...352L..36F.
- ↑ 4.0 4.1 D. A., Gadotti et al. (September 2001), "Homogenization of the Stellar Population along Late-Type Spiral Galaxies", The Astronomical Journal 122 (3): 1298–1318, arXiv:astro-ph/0106303, Bibcode:2001AJ....122.1298G, doi:10.1086/322126.
- ↑ 5.0 5.1 Aranda, Ted (2012), 3,000 Deep-Sky Objects: An Annotated Catalogue, Patrick Moore's practical astronomy series, Springer, p. 107, ISBN 144199419X.
- ↑ Buta, Ronald J. et al. (2007), Atlas of Galaxies, Cambridge University Press, pp. 13–17, ISBN 0521820480.
- ↑ D. W. E., Green, ed. (July 2006), "Supernova 2006dr in NGC 1288", Central Bureau Electronic Telegrams 578: 1, Bibcode:2006CBET..578....1M.
- ↑ B., Monard (June 2007), "Report on CCD activities at the Bronberg Observatory (CBA Pretoria) in 2006", Monthly Notes of the Astronomical Society of South Africa 66 (5–6): 106–109, Bibcode:2007MNSSA..66..106M.
External links
Wikimedia Commons has media related to NGC 1288. |
- Nemiroff, Robert et al. (December 30, 1999), "The Century that Defined Galaxy", Astronomy Picture of the Day (NASA), retrieved 2013-07-08.
- FORS1 First Light - Spiral galaxy NGC 1288, ESO, September 23, 1998, retrieved 2013-07-08.
Coordinates: 03h 17m 13.176s, −32° 34′ 33.08″