UGC 4879
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UGC 4879 | |
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![]() UGC 4879, taken using Hubble's Advanced Camera for Surveys | |
Observation data (J2000 epoch) | |
Constellation | Columba |
Right ascension | 09h 16m 02.023s[1] |
Declination | +52° 50′ 42.05″[1] |
Redshift | -0.000233[2] |
Helio radial velocity | -70[2] |
Distance | 4.18 ± 0.41 Mly (1.283 ± 0.126 Mpc)[2] |
Group or cluster | Local Group |
Apparent magnitude (V) | 13.2[3] |
Apparent magnitude (B) | 14.0[3] |
Characteristics | |
Type | IAm[2] |
Size | 3,000 ly (930 pc)[2] |
Apparent size (V) | 2.5′ × 1.5′[2] |
Notable features | Isolated dwarf galaxy in the Local Group |
Other designations | |
VV 124, MGC+09-15-113, PGC 26124[3] | |
UGC 4879, which is also known as VV 124, is the most isolated dwarf galaxy in the periphery of the Local Group. It is an irregular galaxy at a distance of 1.38 Mpc. Low-resolution spectroscopy yielded inconsistent radial velocities for different components of the galaxy, hinting at the presence of a stellar disk. There is also evidence of this galaxy containing dark matter.
Appearance
UGC 4879 is a transition type galaxy, meaning it has no rings (Denoted rs). It is also a spheroidal (dSph) galaxy, meaning it has a low luminosity. It has little to no gas or dust, or recent star formation. It is also irregular, meaning it has no specific form.[4]
Gallery
References
- ↑ 1.0 1.1 Adelman-McCarthy, J. K. (2009). "VizieR Online Data Catalog: The SDSS Photometric Catalog, Release 7". VizieR On-line Data Catalog. Bibcode 2009yCat.2294....0A.
- ↑ 2.0 2.1 2.2 2.3 2.4 2.5 Lua error in Module:Citation/CS1 at line 379: attempt to call method 'match' (a nil value).
- ↑ 3.0 3.1 3.2 Lua error in Module:Citation/CS1 at line 379: attempt to call method 'match' (a nil value).
- ↑ VV124 (UGC4879): A new transitional dwarf galaxy in the periphery of the Local Group. arXiv:0803.1107. Bibcode 2008MNRAS.387L..45K. doi:10.1111/j.1745-3933.2008.00482.x.
- ↑ Lua error in Module:Citation/CS1 at line 379: attempt to call method 'match' (a nil value).