| NGC 5829 | |
|---|---|
 NGC 5829 by SDSS | |
| Observation data (J2000 epoch) | |
| Constellation | Boötes |
| Right ascension | 15h 02m 42.0s[1] |
| Declination | +23° 20′ 00.0″[1] |
| Redshift | 0.018797[1] |
| Apparent magnitude (V) | 14.1[1] |
| Characteristics | |
| Type | SA(s)c[1] |
| Apparent size (V) | 81.20″ by 63.64″[1] |
| Notable features | Interacting with the galaxy IC 4526 |
| Other designations | |
| VV 7, LEDA 53709, Z 134-70, Arp 42, 2MASX J15024196+2320009, UGC 9673, HCG 73a, MCG+04-35-027, Z 1500.4+2331, CGCG 134.070, PGC 53709 | |
NGC 5829 is a spiral galaxy located in the constellation Boötes. It is 281 million light-years away from Earth and was discovered by astronomer, Edouard Stephan in May 1882.[2]
The luminosity class of NGC 5829 is III and it has an HI line with regions of ionized hydrogen.[3] With a surface brightness of only 14.42 magnitude, NGC 5829 can be classified as a low-surface brightness galaxy.[4]
NGC 5829 forms a galaxy pair Arp 42 with the irregular galaxy IC 4526.[5] Although interacting, the two are not close since IC 4526 is located at a much further distance at 665 million light-years compared to NGC 5829.[6]
- ^ a b c d e f "NASA/IPAC Extragalactic Database". Results for NGC 5829. Retrieved 7 October 2014.
- ^ "New General Catalog Objects: NGC 5800 - 5849". cseligman.com. Retrieved 2024-07-19.
- ^ Springob, Christopher M.; Haynes, Martha P.; Giovanelli, Riccardo; Kent, Brian R. (2005-09-01). "A Digital Archive of H I 21 Centimeter Line Spectra of Optically Targeted Galaxies". The Astrophysical Journal Supplement Series. 160: 149–162. doi:10.1086/431550. ISSN 0067-0049.
- ^ "Revised NGC and IC Catalogue data from Wolfgang Steinickle, from NGC 5800 to 5899". astrovalleyfield.ca. Retrieved 2024-07-19.
- ^ Arp, Halton (1966-11-01). "Atlas of Peculiar Galaxies". The Astrophysical Journal Supplement Series. 14: 1. doi:10.1086/190147. ISSN 0067-0049.
- ^ "NED Search results for IC 4526". ned.ipac.caltech.edu. Retrieved 2024-07-19.