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The pairwise velocity difference of over 2000 BHB stars in the Milky Way halo
Xue, Xiang-Xiang1,2,3; Rix, Hans-Walter2; Zhao, Gang1
2009-11-01
Source PublicationRESEARCH IN ASTRONOMY AND ASTROPHYSICS
Volume9Issue:11Pages:1230-1240
AbstractModels of hierarchical galaxy formation predict that the extended stellar halos of galaxies like our Milky Way show a great deal of sub-structure, arising from disrupted satellites. Spatial sub-structure is directly observed, and has been quantified, in the Milky Way's stellar halo. Phase-space conservation implies that there should be sub-structure in position-velocity space. Here, we aim to quantify such position-velocity sub-structure, using a state-of-the art data set having over 2000 blue horizontal branch (BHB) stars with photometry and spectroscopy from SDSS. For stars in dynamically cold streams ("young" streams), we expect that pairs of objects that are physically close also have similar velocities. Therefore, we apply the well-established "pairwise velocity difference" (PVD) statistic (Delta r), where we expect to drop for small separations Delta r. We calculate the PVD for the SDSS BHB sample and find (Delta r) approximate to const., i.e. no such signal. By making mock-observations of the simulations by Bullock Johnston and applying the same statistic, we show that for individual, dynamically young streams, or assemblages of such streams, drops for small distance separations Delta r, as qualitatively expected. However, for a realistic complete set of halo streams, the pair-wise velocity difference shows no signal, as the simulated halos are dominated by "dynamically old" phase-mixed streams. Our findings imply that the sparse sampling and the sample sizes in SDSS DR6 are still insufficient to use the position-velocity sub-structure for a stringent quantitative data-model comparison. Therefore, alternate statistics must be explored and much more densely sampled surveys, dedicated to the structure of the Milky Way, such as LAMOST, are needed.
KeywordCosmology: Dark Matter Galaxies: Individual (Milky Way) Galaxy: Halo Stars: Horizontal-branch Stars: Kinematics
Indexed BySCI
Language英语
WOS IDWOS:000272605700006
Citation statistics
Cited Times:5[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/7936
Collection光学天文研究部
Affiliation1.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
2.Max Planck Inst Astron, D-69117 Heidelberg, Germany
3.Chinese Acad Sci, Grad Univ, Beijing 100049, Peoples R China
Recommended Citation
GB/T 7714
Xue, Xiang-Xiang,Rix, Hans-Walter,Zhao, Gang. The pairwise velocity difference of over 2000 BHB stars in the Milky Way halo[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2009,9(11):1230-1240.
APA Xue, Xiang-Xiang,Rix, Hans-Walter,&Zhao, Gang.(2009).The pairwise velocity difference of over 2000 BHB stars in the Milky Way halo.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,9(11),1230-1240.
MLA Xue, Xiang-Xiang,et al."The pairwise velocity difference of over 2000 BHB stars in the Milky Way halo".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 9.11(2009):1230-1240.
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