UGC 4879
Dwarf Galaxy at the periphery of the Local Group
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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.
Right ascension09h 16m 02.023s[1]
Declination+52° 50′ 42.05″[1]
| UGC 4879 | |
|---|---|
UGC 4879, taken using the Hubble Space Telescope's Advanced Camera for Surveys | |
| Observation data (J2000 epoch) | |
| Constellation | Ursa Major |
| Right ascension | 09h 16m 02.023s[1] |
| Declination | +52° 50′ 42.05″[1] |
| Redshift | −0.000233[2] |
| Heliocentric 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 26142[3] | |
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, and little recent star formation. It is also irregular, meaning it has no specific form.[4]
Gallery
Ground-based observation of UGC 4879 with the legacy surveys
