A combination of SPH and N-body2 for gas dynamics in star clusters

Details A combination of SPH and N-body2 for gas dynamics in star clusters A combination of SPH and N-body2 for gas dynamics in star clusters

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.170..221t&link_type=abstract

(IAU, European Regional Astronomy Meeting, 11th, La Laguna, Spain, July 3-8, 1989) Astrophysics and Space Science (ISSN 0004-640

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Computational Astrophysics, Gas Dynamics, Hydrodynamics, Star Clusters, Star Formation, Astronomical Catalogs, Equations Of Motion, Interstellar Gas, Many Body Problem, Molecular Clouds

Scientific paper

When stars are being formed in a region of a molecular cloud, the presence of the gas of this cloud will influence the dynamics of these newly formed stars. An implementation of Smooth Particle Hydrodynamics within the framework of N-body2, which will permit the study of this kind of mixed systems is discussed. Various gas removal processes are included, and their influence on the behavior of stars and gas is studied.

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