The lower mass function of the young open cluster Blanco 1: from 30 M$\mathsf{_{Jup}}$ to 3 M$\mathsf{_{\odot}}$-Reference-Cited by-同舟云学术

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The lower mass function of the young open cluster Blanco 1: from 30 M$\mathsf{_{Jup}}$ to 3 M$\mathsf{_{\odot}}$

Published:2007-06-18 Issue:2 Volume:471 Page:499-513
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Moraux E.,Bouvier J.,Stauffer J. R.,Barrado y Navascués D.,Cuillandre J.-C.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361:20066308/pdf

Reference66 articles.

1. Photometric study of Zeta SCULPTORIS cluster

2. Brown dwarf populations in open clusters

3. The Limiting Effects of Dust in Brown Dwarf Model Atmospheres

4. Allen, L., Megeath, S. T., Gutermuth, R., et al. 2006, Protostars and Planets V, to appear [arXiv:astro-ph/0603096]

5. Ballesteros-Paredes, J., Klessen, R. S., Mac Low, M.-M., & Vazquez-Semadeni, E. 2006, Protostars and Planets V, to appear [arXiv:astro-ph/0603357]

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