NGC 7199 is a barred spiral galaxy registered in the New General Catalogue. It is located in the direction of the Indus constellation. It was discovered by the English astronomer John Herschel in 1835 using a 47.5 cm (18.7 inch) reflector.[5][6][7][8]
| NGC 7199 | |
|---|---|
 | |
| Observation data (J2000 epoch) | |
| Constellation | Indus |
| Right ascension | 22h 08m 29.84816s[1] |
| Declination | −64° 42′ 21.9257″[1] |
| Redshift | 0.009609[2] |
| Heliocentric radial velocity | 2867 km/s[2] |
| Distance | 130.1 Mly (39.90 Mpc)[3] |
| Apparent magnitude (V) | 13.22[2] |
| Apparent magnitude (B) | 13.87[2] |
| Characteristics | |
| Type | SB(r)a[4] |
| Other designations | |
| PGC 68124[2] | |
See also
editReferences
edit- ^ a b Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051.
- ^ a b c d e "NGC 7199". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-02-04.
- ^ Crook, Aidan C.; Huchra, John P.; Martimbeau, Nathalie; Masters, Karen L.; Jarrett, Tom; Macri, Lucas M. (2007). "Groups of Galaxies in the Two Micron All Sky Redshift Survey". The Astrophysical Journal. 655 (2): 790–813. arXiv:astro-ph/0610732. Bibcode:2007ApJ...655..790C. doi:10.1086/510201. S2CID 11672751.
- ^ "Results for object NGC 7199 (NGC 7199)". NASA/IPAC Extragalactic Database. California Institute of Technology. Retrieved 2021-02-04.
- ^ "NGC 7199". spider.seds.org. Retrieved 2019-01-10.
- ^ "NGC 7199". sim-id. Retrieved 2019-01-10.
- ^ "VizieR". vizier.u-strasbg.fr. Retrieved 2019-01-10.
- ^ "NASA/IPAC Extragalactic Database". ned.ipac.caltech.edu. Retrieved 2019-01-10.
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