中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
A New Hyper-runaway Star Discovered from LAMOST and Gaia: Ejected Almost in the Galactic Rotation Direction

文献类型:期刊论文

作者Li, Yin-Bi1; Luo, A-Li1; Zhao, Gang1; Lu, You-Jun1; Zhang, Xue-Sen2; Zhang, Fu-Peng3; Du, Bing1; Zuo, Fang1; Zhang, Lan1; Huang, Yang4,6
刊名ASTRONOMICAL JOURNAL
出版日期2018-09-01
卷号156期号:3
关键词Galaxy: Center Galaxy: Halo Galaxy: Kinematics And Dynamics Stars: Early-type
ISSN号0004-6256
DOI10.3847/1538-3881/aad09a
产权排序第5完成单位
文献子类Article
英文摘要

In this paper, we report the discovery of a new late-B-type unbound hyper-runaway star (LAMOST-HVS4) from the LAMOST spectroscopic surveys. According to its atmospheric parameters, it is either a B-type main-sequence (MS) star or a blue horizontal branch (BHB) star. Its Galactocentric distance and velocity are 30.3 +/- 1.6 kpc and 586 +/- 7 km s(-1) if it is an MS star, and they are 13.2 +/- 3.7 kpc and 590 +/- 7 km s(-1) if a BHB star. We track its trajectories back and find that the trajectories intersect with the Galactic disk, and the Galactic center lies outside of the intersection region at the 3a confidence level. We investigate a number of mechanisms that could be responsible for the ejection of the star and find that it is probably ejected from the Galactic disk by supernova explosion or multiple-body interactions in dense young stellar clusters.

学科主题天文学
URL标识查看原文
出版地TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
WOS关键词Horizontal-branch Stars ; Sky Survey 2mass ; 1st Data Release ; Hypervelocity Stars ; Black-hole ; Local Standard ; O-star ; Mass ; Origin ; Halo
资助项目National Basic Research Program of China (973 Program)[2014CB845700] ; National Natural Science Foundation of China[11390371/2/4] ; National Science Foundation of China (NSFC)[11773033] ; Astronomical Big Data Joint Research Center ; Alibaba Cloud ; National Development and Reform Commission
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:000441303000004
出版者IOP PUBLISHING LTD
资助机构National Basic Research Program of China (973 Program)[2014CB845700] ; National Natural Science Foundation of China[11390371/2/4] ; National Science Foundation of China (NSFC)[11773033] ; Astronomical Big Data Joint Research Center ; Alibaba Cloud ; National Development and Reform Commission
源URL[http://ir.ynao.ac.cn/handle/114a53/17383]  
专题云南天文台_大样本恒星演化研究组
云南天文台_中国科学院天体结构与演化重点实验室
通讯作者Luo, A-Li; Zhao, Gang; Lu, You-Jun
作者单位1.Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, People's Republic of China
2.ExtantFuture (Beijing)Technology Co., Ltd, Beijing 100102, People's Republic of China
3.School of physics and astronomy, Sun Yat-sen University, Guangzhou 510275, People's Republic of China
4.South-Western Institute for Astronomy Research, Yunnan University, Kunming 650500, People's Republic of China
5.Key Laboratory for the Structure and Evolution of Celestial Objects, Yunnan Observatories,Chinese Academy of Sciences, Kunming 650216, People's Republic of China
6.LAMOST Fellow.
推荐引用方式
GB/T 7714
Li, Yin-Bi,Luo, A-Li,Zhao, Gang,et al. A New Hyper-runaway Star Discovered from LAMOST and Gaia: Ejected Almost in the Galactic Rotation Direction[J]. ASTRONOMICAL JOURNAL,2018,156(3).
APA Li, Yin-Bi.,Luo, A-Li.,Zhao, Gang.,Lu, You-Jun.,Zhang, Xue-Sen.,...&Han ZW.(2018).A New Hyper-runaway Star Discovered from LAMOST and Gaia: Ejected Almost in the Galactic Rotation Direction.ASTRONOMICAL JOURNAL,156(3).
MLA Li, Yin-Bi,et al."A New Hyper-runaway Star Discovered from LAMOST and Gaia: Ejected Almost in the Galactic Rotation Direction".ASTRONOMICAL JOURNAL 156.3(2018).

入库方式: OAI收割

来源:云南天文台

浏览0
下载0
收藏0
其他版本

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。