期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 516, 期 1, 页码 731-748出版社
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stac2036
关键词
stars: individual: BHB; stars: individual: K giants; galaxies: individual: Milky Way; stars: kinematics and dynamics; Galaxy: halo; Galaxy: kinematics and dynamics; Galaxy: stellar content
资金
- National Natural Science Foundation of China [11890694, 11873057, 11873052, 12025302, 11873034, 11988101, 11773052, 11761131016]
- National Key Research and Development Program of China [2018YFA0404501]
- China Manned Space Project [CMS-CSST-2021-B03]
- China Space Station Telescope Milky Way and Nearby Galaxies Survey on Dust and Extinction Project [CMS-CSST-2021-A09, CMS-CSST-2021-A08]
- 111 Project of the Ministry of Education of China [B20019]
- Hubei Provincial Outstanding Youth Fund [2019CFA087]
- Aliyun Fellowship, Chinese Academy of Sciences President's International Fellowship Initiative [2016PE010, 2021PM0055]
- Postdoctoral Scholar's Fellowship of LAMOST
- National Development and Reform Commission
- Alfred P. Sloan Foundation
- National Science Foundation
- U.S. Department of Energy Office of Science
- University of Arizona
- Brazilian Participation Group
- Brookhaven National Laboratory
- Carnegie Mellon University
- University of Florida
- French Participation Group
- German Participation Group
- Harvard University
- Instituto de Astrofisica de Canarias
- Michigan State/Notre Dame/JINA Participation Group
- Johns Hopkins University
- Lawrence Berkeley National Laboratory
- Max Planck Institute for Astrophysics
- Max Planck Institute for Extraterrestrial Physics
- New Mexico State University
- New York University
- Ohio State University
- Pennsylvania State University
- University of Portsmouth
- Princeton University
- Spanish Participation Group
- University of Tokyo
- University of Utah
- Vanderbilt University
- University of Virginia
- University of Washington
- Yale University
Using stellar halo samples, this study estimates the mass distribution and dark matter mass of the Milky Way through two methods. The results show reasonable consistency across different samples and methods.
We measure the enclosed Milky Way mass profile to Galactocentric distances of similar to 70 and similar to 50 kpc using the smooth, diffuse stellar halo samples of Bird et al. The samples are Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) and Sloan Digital Sky Survey/Sloan Extension for Galactic Understanding and Exploration (SDSS/SEGUE) K giants (KG) and SDSS/SEGUE blue horizontal branch (BHB) stars with accurate metallicities. The 3D kinematics are available through LAMOST and SDSS/SEGUE distances and radial velocities and Gaia DR2 proper motions. Two methods are used to estimate the enclosed mass: 3D spherical Jeans equation and Evans et al. tracer mass estimator (TME). We remove substructure via the Xue et al. method based on integrals of motion. We evaluate the uncertainties on our estimates due to random sampling noise, systematic distance errors, the adopted density profile, and non-virialization and non-spherical effects of the halo. The tracer density profile remains a limiting systematic in our mass estimates, although within these limits we find reasonable agreement across the different samples and the methods applied. Out to similar to 70 and similar to 50 kpc, the Jeans method yields total enclosed masses of 4.3 +/- 0.95 (random) +/- 0.6 (systematic) x 10(11) M-circle dot and 4.1 +/- 1.2 (random) +/- 0.6 (systematic) x 10(11) M-circle dot for the KG and BHB stars, respectively. For the KG and BHB samples, we find a dark matter virial mass of M-200 = 0.55(-0.11)(+0.15) (random) +/- 0.083 (systematic) x 10(12) M-circle dot and M-200 = 1.00(-0.33)(+0.67) (random) +/- 0.15 (systematic) x 10(12) M-circle dot, respectively.
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