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Title:
The Properties of Stars and Brown Dwarfs
Authors:
Bate, M. R.; Bonnell, I. A.; Bromm, V.
Affiliation:
AA(School of Physics, University of Exeter, Exeter EX4 4QL, United Kingdom), AB(School of Physics and Astronomy, University of St Andrews, North Haugh, St Andrews, Fife, KY16 9SS, United Kingdom), AC(Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA)
Publication:
In Galactic Star Formation Across the Stellar Mass Spectrum, ASP Conference Series, Vol. 287, proceedings of the 2002 International Astronomical Observatories in Chile workshop, held 11-15 March 2002 at La Serena, Chile. Edited by James M. De Buizer and Nicole S. van der Bliek. San Francisco: Astronomical Society of the Pacific, ISBN: 1-58381-130-3, 2003, p. 427-432
Publication Date:
00/2003
Origin:
ADS; AUTHOR
Comment:
ISBN: 1-58381-130-3
Bibliographic Code:
2003ASPC..287..427B

Abstract

We present results from the most ambitious hydrodynamic star formation calculation performed to date. The calculation follows the collapse and fragmentation of a large scale turbulent molecular cloud to form a stellar association consisting of dozens of stars and brown dwarfs. It resolves all fragmentation down to the opacity limit, binary stars with separations as small as 1 AU, and circumstellar discs with radii down to ≈ 10 AU. For the first time, the combination of high resolution and the large number of objects formed allows us to compare a wide variety of statistical properties with those observed in star forming regions.

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