Constraining the Stellar Mass Function in the Galactic Center via Mass Loss from Stellar Collisions

The dense concentration of stars and high-velocity dispersions in the Galactic center imply that stellar collisions frequently occur. Stellar collisions could therefore result in significant mass loss rates. We calculate the amount of stellar mass lost due to indirect and direct stellar collisions a...

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Main Authors: Douglas Rubin, Abraham Loeb
Format: Article
Language:English
Published: Wiley 2011-01-01
Series:Advances in Astronomy
Online Access:http://dx.doi.org/10.1155/2011/174105
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author Douglas Rubin
Abraham Loeb
author_facet Douglas Rubin
Abraham Loeb
author_sort Douglas Rubin
collection DOAJ
description The dense concentration of stars and high-velocity dispersions in the Galactic center imply that stellar collisions frequently occur. Stellar collisions could therefore result in significant mass loss rates. We calculate the amount of stellar mass lost due to indirect and direct stellar collisions and find its dependence on the present-day mass function of stars. We find that the total mass loss rate in the Galactic center due to stellar collisions is sensitive to the present-day mass function adopted. We use the observed diffuse X-ray luminosity in the Galactic center to preclude any present-day mass functions that result in mass loss rates >10-5M⨀yr−1 in the vicinity of ~1″. For present-day mass functions of the form, dN/dM∝M-α, we constrain the present-day mass function to have a minimum stellar mass ≲7M⨀ and a power-law slope ≳1.25. We also use this result to constrain the initial mass function in the Galactic center by considering different star formation scenarios.
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spelling doaj-art-54bcdf91e5a145f89e572651873cae412025-08-20T02:05:07ZengWileyAdvances in Astronomy1687-79691687-79772011-01-01201110.1155/2011/174105174105Constraining the Stellar Mass Function in the Galactic Center via Mass Loss from Stellar CollisionsDouglas Rubin0Abraham Loeb1Department of Physics, Harvard University, Cambridge, MA 02138, USADepartment of Astronomy, Harvard University, Cambridge, MA 02138, USAThe dense concentration of stars and high-velocity dispersions in the Galactic center imply that stellar collisions frequently occur. Stellar collisions could therefore result in significant mass loss rates. We calculate the amount of stellar mass lost due to indirect and direct stellar collisions and find its dependence on the present-day mass function of stars. We find that the total mass loss rate in the Galactic center due to stellar collisions is sensitive to the present-day mass function adopted. We use the observed diffuse X-ray luminosity in the Galactic center to preclude any present-day mass functions that result in mass loss rates >10-5M⨀yr−1 in the vicinity of ~1″. For present-day mass functions of the form, dN/dM∝M-α, we constrain the present-day mass function to have a minimum stellar mass ≲7M⨀ and a power-law slope ≳1.25. We also use this result to constrain the initial mass function in the Galactic center by considering different star formation scenarios.http://dx.doi.org/10.1155/2011/174105
spellingShingle Douglas Rubin
Abraham Loeb
Constraining the Stellar Mass Function in the Galactic Center via Mass Loss from Stellar Collisions
Advances in Astronomy
title Constraining the Stellar Mass Function in the Galactic Center via Mass Loss from Stellar Collisions
title_full Constraining the Stellar Mass Function in the Galactic Center via Mass Loss from Stellar Collisions
title_fullStr Constraining the Stellar Mass Function in the Galactic Center via Mass Loss from Stellar Collisions
title_full_unstemmed Constraining the Stellar Mass Function in the Galactic Center via Mass Loss from Stellar Collisions
title_short Constraining the Stellar Mass Function in the Galactic Center via Mass Loss from Stellar Collisions
title_sort constraining the stellar mass function in the galactic center via mass loss from stellar collisions
url http://dx.doi.org/10.1155/2011/174105
work_keys_str_mv AT douglasrubin constrainingthestellarmassfunctioninthegalacticcenterviamasslossfromstellarcollisions
AT abrahamloeb constrainingthestellarmassfunctioninthegalacticcenterviamasslossfromstellarcollisions