A new Monte Carlo method for dynamical evolution of non-spherical stellar systems
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/446/3/3150/10448436/stu2360.pdf
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1. STRONG MASS SEGREGATION AROUND A MASSIVE BLACK HOLE
2. Accretion of stars on to a massive black hole: a realistic diffusion model and numerical studies
3. ON THE DISTRIBUTION OF STELLAR REMNANTS AROUND MASSIVE BLACK HOLES: SLOW MASS SEGREGATION, STAR CLUSTER INSPIRALS, AND CORRELATED ORBITS
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