fbpx
Wikipedia

UGC 4879

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.

UGC 4879
Observation data (J2000 epoch)
ConstellationUrsa Major
Right ascension09h 16m 02.023s[1]
Declination+52° 50′ 42.05″[1]
Redshift-0.000233[2]
Heliocentric radial velocity-70[2]
Distance4.18 ± 0.41 Mly (1.283 ± 0.126 Mpc)[2]
Group or clusterLocal Group
Apparent magnitude (V)13.2[3]
Apparent magnitude (B)14.0[3]
Characteristics
TypeIAm[2]
Size3,000 ly (930 pc)[2]
Apparent size (V)2.5 × 1.5[2]
Notable featuresIsolated dwarf galaxy in the Local Group
Other designations
VV 124, MGC+09-15-113, PGC 26142[3]

Appearance edit

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 edit

References edit

  1. ^ a b Adelman-McCarthy, J. K.; et al. (2009). "VizieR Online Data Catalog: The SDSS Photometric Catalog, Release 7". VizieR On-line Data Catalog. Bibcode:2009yCat.2294....0A.
  2. ^ a b c d e f "NED results for object UGC 4879". National Aeronautics and Space Administration / Infrared Processing and Analysis Center. Retrieved 19 February 2017.
  3. ^ a b c "UGC 4879". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 19 February 2017.
  4. ^ Kopylov, A. I.; Tikhonov, N. A.; Fabrika, S.; Drozdovsky, I.; Valeev, A. F. (2008). "VV124 (UGC4879): A new transitional dwarf galaxy in the periphery of the Local Group". Monthly Notices of the Royal Astronomical Society: Letters. 387 (1): L45–L49. arXiv:0803.1107. Bibcode:2008MNRAS.387L..45K. doi:10.1111/j.1745-3933.2008.00482.x. S2CID 17166212.
  5. ^ "A mysterious hermit". Retrieved 8 June 2016.

External links edit

  • C2.staticflickr.com

4879, which, also, known, most, isolated, dwarf, galaxy, periphery, local, group, irregular, galaxy, distance, resolution, spectroscopy, yielded, inconsistent, radial, velocities, different, components, galaxy, hinting, presence, stellar, disk, there, also, ev. 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 UGC 4879UGC 4879 taken using the Hubble Space Telescope s Advanced Camera for SurveysObservation data J2000 epoch ConstellationUrsa MajorRight ascension09h 16m 02 023s 1 Declination 52 50 42 05 1 Redshift 0 000233 2 Heliocentric radial velocity 70 2 Distance4 18 0 41 Mly 1 283 0 126 Mpc 2 Group or clusterLocal GroupApparent magnitude V 13 2 3 Apparent magnitude B 14 0 3 CharacteristicsTypeIAm 2 Size3 000 ly 930 pc 2 Apparent size V 2 5 1 5 2 Notable featuresIsolated dwarf galaxy in the Local GroupOther designationsVV 124 MGC 09 15 113 PGC 26142 3 Contents 1 Appearance 2 Gallery 3 References 4 External linksAppearance editUGC 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 edit nbsp There are about 2 3 million light years between UGC 4879 and its closest neighbour Leo A 5 References edit a b Adelman McCarthy J K et al 2009 VizieR Online Data Catalog The SDSS Photometric Catalog Release 7 VizieR On line Data Catalog Bibcode 2009yCat 2294 0A a b c d e f NED results for object UGC 4879 National Aeronautics and Space Administration Infrared Processing and Analysis Center Retrieved 19 February 2017 a b c UGC 4879 SIMBAD Centre de donnees astronomiques de Strasbourg Retrieved 19 February 2017 Kopylov A I Tikhonov N A Fabrika S Drozdovsky I Valeev A F 2008 VV124 UGC4879 A new transitional dwarf galaxy in the periphery of the Local Group Monthly Notices of the Royal Astronomical Society Letters 387 1 L45 L49 arXiv 0803 1107 Bibcode 2008MNRAS 387L 45K doi 10 1111 j 1745 3933 2008 00482 x S2CID 17166212 A mysterious hermit Retrieved 8 June 2016 External links edit nbsp Wikimedia Commons has media related to UGC 4879 C2 staticflickr com Retrieved from https en wikipedia org w index php title UGC 4879 amp oldid 1162440404, wikipedia, wiki, book, books, library,

article

, read, download, free, free download, mp3, video, mp4, 3gp, jpg, jpeg, gif, png, picture, music, song, movie, book, game, games.