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The RAVE survey: constraining the local Galactic escape speed

Smith, Martin C.; Ruchti, Gregory R.; Helmi, Amina; Wyse, Rosemary F. G.; Fulbright, J. P.; Freeman, K. C.; Navarro, J. F.; Seabroke, G. M.; Steinmetz, M.; Williams, M.; Bienaymé, O.; Binney, J.; Bland-Hawthorn, J.; Dehnen, W.; Gibson, B. K.; Gilmore, G.; Grebel, E. K.; Munari, U.; Parker, Q. A.; Scholz, R.-D.; Siebert, A.; Watson, F. G. and Zwitter, T. (2007). The RAVE survey: constraining the local Galactic escape speed. Monthly Notices of the Royal Astronomical Society, 379(2) p. 755.

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DOI (Digital Object Identifier) Link: https://doi.org/10.1111/j.1365-2966.2007.11964.x
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Abstract

We report new constraints on the local escape speed of our Galaxy. Our analysis is based on a sample of high-velocity stars from the RAVE survey and two previously published data sets. We use cosmological simulations of disc galaxy formation to motivate our assumptions on the shape of the velocity distribution, allowing for a significantly more precise measurement of the escape velocity compared to previous studies. We find that the escape velocity lies within the range 498 < vesc < 608 km s?1 (90 per cent confidence), with a median likelihood of 544 km s?1. The fact that v2esc is significantly greater than 2v2circ (where vcirc= 220 km s?1 is the local circular velocity) implies that there must be a significant amount of mass exterior to the solar circle, that is, this convincingly demonstrates the presence of a dark halo in the Galaxy. We use our constraints on vesc to determine the mass of the Milky Way halo for three halo profiles. For example, an adiabatically contracted NFW halo model results in a virial mass of 1.42+1.14?0.54× 1012 M? and virial radius of (90 per cent confidence). For this model the circular velocity at the virial radius is 142+31?21 km s?1. Although our halo masses are model dependent, we find that they are in good agreement with each other.

Item Type: Journal Item
ISSN: 1365-2966
Extra Information: Some of the symbols may not have transferred correctly into this bibliographic record and/or abstract.
Academic Unit/School: Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
Item ID: 12967
Depositing User: George Seabroke
Date Deposited: 04 Feb 2009 06:29
Last Modified: 03 May 2019 15:35
URI: http://oro.open.ac.uk/id/eprint/12967
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