From Molecular Cores to Stars and Brown Dwarfs

Details From Molecular Cores to Stars and Brown Dwarfs From Molecular Cores to Stars and Brown Dwarfs

Aug 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ap%26ss.292..297b&link_type=abstract

Astrophysics and Space Science, v. 292, Issue 1, p. 297-307 (2004).

Astronomy and Astrophysics

Astrophysics

1

Accretion, Accretion Discs, Binaries: General, Brown Dwarfs, Hydrodynamics, Stars: Formation

Scientific paper

In this paper, we review the results from numerical simulations that investigate the evolution of molecular cores into stars and brown dwarfs. We begin by discussing the four main processes involved in this evolution, fragmentation, accretion, interactions with discs, and stellar dynamical interactions. We then discuss large-scale calculations in which all of these processes are model simultaneously. Finally, we review results that have been obtained from past magnetohydrodynamical (MHD) calculations of fragmentation and look towards future MHD calculations.

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