On kinematic substructure in the Sextans dwarf spheroidal galaxy

被引:64
作者
Walker, MG
Mateo, M
Olszewski, EW
Pal, JK
Sen, B
Woodroofe, M
机构
[1] Univ Michigan, Dept Astron, Ann Arbor, MI 48109 USA
[2] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA
[3] Univ Michigan, Dept Stat, Ann Arbor, MI 48109 USA
关键词
galaxies : dwarf; galaxies : individual (Sextans); galaxies : kinematics and dynamics; Local Group;
D O I
10.1086/504522
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present multifiber echelle radial velocity results for 551 stars in the Sextans dwarf spheroidal galaxy and identify 294 stars as probable Sextans members. The projected velocity dispersion profile of the binned data remains flat to a maximum angular radius of 30'. We introduce a nonparametric technique for estimating the projected velocity dispersion surface and use this to search for kinematic substructure. Our data do not confirm previous reports of a kinematically distinct stellar population at the Sextans center. Instead we detect a region near the Sextans core radius that is kinematically colder than the overall Sextans sample with 95% confidence.
引用
收藏
页码:L41 / L44
页数:4
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