Constraints on the pairing properties of main-sequence stars from observations of white dwarfs in binary systems-Reference-Cited by-同舟云学术

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Constraints on the pairing properties of main-sequence stars from observations of white dwarfs in binary systems

Published:2012-10-15 Issue:3 Volume:426 Page:2500-2506
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Monthly Notices of the Royal Astronomical Society

Author:

Ferrario Lilia¹

Affiliation:

1. Mathematical Sciences Institute; The Australian National University; Canberra; ACT; 0200; Australia

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/426/3/2500/3122383/426-3-2500.pdf

Reference40 articles.

1. Accretion during binary star formation -- I. Ballistic accretion

2. Stellar, brown dwarf and multiple star properties from a radiation hydrodynamical simulation of star cluster formation

3. A COMPREHENSIVE SPECTROSCOPIC ANALYSIS OF DB WHITE DWARFS

4. THE LUMINOSITY AND MASS FUNCTIONS OF LOW-MASS STARS IN THE GALACTIC DISK. II. THE FIELD

5. The formation of close binary systems

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