THE NEAREST HIGH-VELOCITY STARS REVEALED BY LAMOST DATA RELEASE 1

被引:35
|
作者
Zhong, Jing [1 ]
Chen, Li [1 ]
Liu, Chao [2 ]
de Grijs, Richard [3 ,4 ]
Hou, Jinliang [1 ]
Shen, Shiyin [1 ]
Shao, Zhengyi [1 ]
Li, Jing [1 ]
Luo, Ali [2 ]
Shi, Jianrong [2 ]
Zhang, Haotong [2 ]
Yang, Ming [2 ]
Deng, Licai [2 ]
Jin, Ge [5 ]
Zhang, Yong [6 ]
Hou, Yonghui [6 ]
Zhang, Zhenchao [6 ]
机构
[1] Chinese Acad Sci, Shanghai Astron Observ, Key Lab Res Galaxies & Cosmol, 80 Nandan Rd, Shanghai 200030, Peoples R China
[2] Chinese Acad Sci, Natl Astron Observ, Key Lab Opt Astron, Beijing 100012, Peoples R China
[3] Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China
[4] Peking Univ, Dept Astron, Beijing 100871, Peoples R China
[5] Univ Sci & Technol China, Hefei 230026, Peoples R China
[6] Chinese Acad Sci, Natl Astron Observ, Nanjing Inst Astron Opt & Technol, Nanjing 210042, Jiangsu, Peoples R China
基金
中国国家自然科学基金;
关键词
astrometry; Galaxy: halo; Galaxy: structure; stars: kinematics and dynamics; surveys; DIGITAL SKY SURVEY; EXTREME RUNAWAY STAR; MILKY-WAY TOMOGRAPHY; HYPERVELOCITY STAR; PILOT SURVEY; INTERSTELLAR EXTINCTION; GALACTIC-CENTER; BLACK-HOLE; HIP; 60350; LEGUE;
D O I
10.1088/2041-8205/789/1/L2
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the discovery of 28 candidate high-velocity stars (HVSs) at heliocentric distances of less than 3 kpc, based on the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) Data Release 1. Our sample of HVS candidates covers a much broader color range than the equivalent ranges discussed in previous studies and comprises the first and largest sample of HVSs in the immediate solar neighborhood, at heliocentric distances less than 1-3 kpc. The observed as well as the derived parameters for all candidates are sufficiently accurate to allow us to ascertain their nature as genuine HVSs, of which a subset of 12 objects represents the most promising candidates. Our results also highlight the great potential of discovering statistically large numbers of HVSs of different spectral types in LAMOST survey data. This will ultimately enable us to achieve a better understanding of the nature of Galactic HVSs and their ejection mechanisms, and to constrain the structure of the Galaxy.
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页数:7
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