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Minimum Mass of Brown Dwarfs

Published online by Cambridge University Press:  26 May 2016

Taishi Nakamoto
Affiliation:
University of Tsukuba, Japan
Koji Ogochi
Affiliation:
Information Technology Japan Inc., Japan

Abstract

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We investigate the minimum mass of brown dwarfs using radiation hydrodynamics simulations of collapsing filamentary clouds and analytical estimates. We found the minimum mass of brown dwarfs depends on the initial temperature of parent clouds and the nature of heating sources. The universal minimum mass of brown dwarfs, which is about 0.007M, is given when the initial cloud temperature is 13.3 K. Our results are consistent with recent observations of low-mass objects in some star forming regions.

Type
Part II: Progress in the theory of planet formation
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Hillenbrand, L. A., & Carpenter, J. M. 2000, ApJ, 540, 236.CrossRefGoogle Scholar
Inutsuka, S., & Miyama, S. M. 1997, ApJ, 480, 681 (IM97).Google Scholar
Luhman, K. L., Rieke, G. H., Young, T., Cotera, A. S., Chen, H., Rieke, M. J., Schneider, G., & Thompson, R. I. 2000, ApJ, 540, 1016.CrossRefGoogle Scholar
Masunaga, H., & Inutsuka, S. 1999, ApJ, 510, 822.CrossRefGoogle Scholar
Miyama, S. M., Narita, S., & Hayashi, C. 1984, Prog. Theor. Phys., 78, 1273.Google Scholar
Ogochi, K., & Nakamoto, T. 2000, ApJ, submitted.Google Scholar
Rees, M. 1976, MNRAS, 176, 483.Google Scholar
Silk, J. 1977, ApJ, 214, 152.Google Scholar
Zapatero Osorio, M. R., Béjar, V. J. S., Rebolo, R., Martin, E. L., & Basri, G. 1999, ApJ, 524, L115.Google Scholar