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Joint constraints on the Galactic dark matter halo and GC from hypervelocity stars

Rossi, E. M. and Marchetti, T. and Cacciato, M. and Kuiack, M. and Sari, R. (2017) Joint constraints on the Galactic dark matter halo and GC from hypervelocity stars. Monthly Notices of the Royal Astronomical Society, 467 (2). pp. 1844-1856. ISSN 0035-8711. http://resolver.caltech.edu/CaltechAUTHORS:20170428-075210118

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Abstract

The mass assembly history of the Milky Way can inform both theory of galaxy formation and the underlying cosmological model. Thus, observational constraints on the properties of both its baryonic and dark matter contents are sought. Here, we show that hypervelocity stars (HVSs) can in principle provide such constraints. We model the observed velocity distribution of HVSs, produced by tidal break-up of stellar binaries caused by Sgr A*. Considering a Galactic Centre (GC) binary population consistent with that inferred in more observationally accessible regions, a fit to current HVS data with significance level >5 per cent can only be obtained if the escape velocity from the GC to 50 kpc is VG ≲ 850 km s^(−1), regardless of the enclosed mass distribution. When a Navarro, Frenk and White matter density profile for the dark matter halo is assumed, haloes with VG ≲ 850 km s^(−1) are in agreement with predictions in the Λ cold dark matter model and a subset of models around M200 ∼ 0.5–1.5 × 10^(12) M_⊙ and rs ≲ 35 kpc can also reproduce Galactic circular velocity data. HVS data alone cannot currently exclude potentials with VG > 850 km s^(−1). Finally, specific constraints on the halo mass from HVS data are highly dependent on the assumed baryonic mass potentials. This first attempt to simultaneously constrain GC and dark halo properties is primarily hampered by the paucity and quality of data. It nevertheless demonstrates the potential of our method, that may be fully realized with the ESA Gaia mission.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1093/mnras/stx098DOIArticle
https://academic.oup.com/mnras/article/467/2/1844/2907759/Joint-constraints-on-the-Galactic-dark-matter-halo?searchresult=1PublisherArticle
https://arxiv.org/abs/1608.02000arXivDiscussion Paper
Additional Information:© 2017 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. Accepted 2017 January 12. Received 2017 January 6; in original form 2016 July 12. We thank S. de Mink and R. Schödel for a careful reading of the manuscript and O. Gnedin, M. Viola, H. Perets, E. Starkenburg, J. Navarro, A. Helmi, S. Kobayashi and A. Brown for useful discussions and comments. We also thank the anonymous referee for the careful reading of the manuscript and his/her useful suggestions. EMR and TM acknowledge the support from NWO TOP grant Module 2, project number 614.001.401.
Group:TAPIR
Funders:
Funding AgencyGrant Number
NWO TOP grant Module 2614.001.401
Subject Keywords:methods: analytical, stars: kinematics and dynamics, - Galaxy: Centre, Galaxy: halo, dark matter
Record Number:CaltechAUTHORS:20170428-075210118
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20170428-075210118
Official Citation:E. M. Rossi, T. Marchetti, M. Cacciato, M. Kuiack, R. Sari; Joint constraints on the Galactic dark matter halo and Galactic Centre from hypervelocity stars. Mon Not R Astron Soc 2017; 467 (2): 1844-1856. doi: 10.1093/mnras/stx098
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:77038
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:28 Apr 2017 16:09
Last Modified:28 Apr 2017 16:09

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