TIDAL DWARF GALAXIES AROUND A POST-MERGER GALAXY, NGC 4922

被引:11
|
作者
Sheen, Yun-Kyeong [1 ]
Jeong, Hyunjin [1 ]
Yi, Sukyoung K. [1 ]
Ferreras, Ignacio [2 ]
Lotz, Jennifer M. [3 ]
Olsen, Knut A. G. [3 ]
Dickinson, Mark [3 ]
Barnes, Sydney [4 ]
Park, Jang-Hyun [5 ]
Ree, Chang H.
Madore, Barry F. [6 ]
Barlow, Tom A. [7 ]
Conrow, Tim [7 ]
Foster, Karl [7 ]
Friendman, Peter G. [7 ]
Lee, Young-Wook [1 ]
Martin, D. Christopher [7 ]
Morrissey, Patrick [7 ]
Neff, Susan G. [8 ]
Schiminovich, David [9 ]
Seibert, Mark [6 ]
Small, Todd [7 ]
Wyder, Ted K. [7 ]
机构
[1] Yonsei Univ, Dept Astron, Seoul 120749, South Korea
[2] Univ Coll London, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England
[3] Natl Opt Astron Observ, Tucson, AZ 85719 USA
[4] Lowell Observ, Flagstaff, AZ 86001 USA
[5] Korea Astron & Space Sci Inst, Taejon 305348, South Korea
[6] Observ Carnegie Inst Washington, Pasadena, CA 91101 USA
[7] CALTECH, Pasadena, CA 91125 USA
[8] NASA, Goddard Space Flight Ctr, Astron & Solar Phys Lab, Greenbelt, MD 20771 USA
[9] Columbia Univ, Dept Astron, New York, NY 10027 USA
来源
ASTRONOMICAL JOURNAL | 2009年 / 138卷 / 06期
关键词
galaxies: dwarf; galaxies: individual (NGC 4922); galaxies: interactions; galaxies: starburst; ultraviolet: galaxies; GLOBULAR-CLUSTER FORMATION; STAR-FORMATION; INTERACTING GALAXIES; EVOLUTION-EXPLORER; TAILS; GAS; CANDIDATE; NGC-4038/39; EMISSION; ANTENNAE;
D O I
10.1088/0004-6256/138/6/1911
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
One possible channel for the formation of dwarf galaxies involves birth in the tidal tails of interacting galaxies. We report the detection of a bright UV tidal tail and several young tidal dwarf galaxy (TDG) candidates in the post-merger galaxy NGC 4922 in the Coma cluster. Based on a two-component population model ( combining young and old stellar populations), we find that the light of tidal tail predominantly comes from young stars (a few Myr old). The Galaxy Evolution Explorer ultraviolet data played a critical role in the parameter (age and mass) estimation. Our stellar mass estimates of the TDG candidates are similar to 10(6-7) M-circle dot, typical for dwarf galaxies.
引用
收藏
页码:1911 / 1916
页数:6
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