A bound on galactic mass loss rates obtaind from globular cluster dynamics

Details A bound on galactic mass loss rates obtaind from globular cluster dynamics A bound on galactic mass loss rates obtaind from globular cluster dynamics

2004-05-11

arxiv.org/abs/astro-ph/0405201v3

Class.Quant.Grav. 21 (2004) 5075

Astronomy and Astrophysics

Astrophysics

7 pages, no figures, replaced with the version accepted for publication: New title, ref. added

Scientific paper

10.1088/0264-9381/21/22/004

Using tidal disruption of globular clusters by the galactic center, we put
limits on the total mass ever enclosed into orbits of observed globular
clusters. Under the assumption that the rate of mass loss from the Galaxy is
steady, we then deduce a bound on this rate. In particular this bound can be
used to constrain the galactic gravitational wave luminosity.

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