The metallicity of K giant stars along the Sagittarius strea

发布时间：2018-04-01 08:23

  本文选题：Galaxy　切入点：halo　出处：《Research in Astronomy and Astrophysics》2017年07期

【摘要】：The Large Sky-Area Multi-Object Fiber Spectroscopic Telescope(LAMOST) Data Release3 provided 341 691 K giant stars with stellar parameters. Based on the models of Law Majewski, we identified 252 K giant stars in the leading stream associated with the Sagittarius(Sgr) dwarf galaxy. We obtained 132 K giant stars belonging to the trailing arm of Sgr using the model of Belokurov et al. We studied the metallicity distribution of member stars along the streams and found a flat gradient in the first wrap of the leading stream, (0.88±0.3) × 10~(-3)dex/(~?) in the second wrap of the leading stream and (1.2±0.3) × 10~(-3)dex/(~?) in the first wrap of the trailing stream. Moreover, we obtained a combined metallicity gradient with our sample and data from the literature. We also analyzed the properties of an overdensity, which is located in the leading stream of the Sgr.
[Abstract]:Data Release3 provided 341,691 K giant stars with stellar parameters. Based on the models of Law Majewski. we identified 252K giant stars in the leading stream stream with the Sagitustarius dwarf Galaxy y. We obtained 132K giant stars belonging to the trailing trailing of the trailing the model of Belokurov et al.We studied the metallicity distribution of distribution of distribution. The streams and found a flat gradient in the first wrap of the leading stream, 0. 88 卤0. 3) 脳 10? In the second wrap of the leading stream and, 1.2 卤0.3) 脳 10 ~ (3) DX / P? ) in the first wrap of the trailing stream.Moreover, we obtained a combined metallicity gradient with our sample and data from from the literature.We also analyzed the properties of an overdensity.#en20# is located in the stream of the Sgr.
【作者单位】： Shandong
【基金】：supported by National Natural Science Foundation of China (Grant Nos. U1631105, 11390371, 11573035, 11233004, 11625313, 11373026, 11303003 and 11673005) the 973 program (No. 2014CB845700) the Strategic Priority Research Program of the Chinese Academy of Sciences (Grant No. XDB01020300)
【分类号】：P152

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