Physical parameters and evolutionary route for the Large Magellanic Cloud interacting binary OGLE 05155332−6925581★-Reference-Cited by-同舟云学术

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Physical parameters and evolutionary route for the Large Magellanic Cloud interacting binary OGLE 05155332−6925581★

Published:2012-10-31 Issue:2 Volume:428 Page:1594-1605
ISSN:1365-2966
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Garrido H. E.,Mennickent R. E.,Djurašević G.,Kołaczkowski Z.,Niemczura E.,Mennekens N.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/428/2/1594/3270880/sts143.pdf

Reference36 articles.

1. Possible gravitational microlensing of a star in the Large Magellanic Cloud

2. Three-dimensional numerical simulation of gaseous flow structure in semidetached binaries

3. The possible nature of dips in the light curves of semidetached binaries with stationary disks

4. A spectroscopic atlas of the HgMn star HD 175640 (B9 V) $\lambda\lambda$ 3040–10 000 Å

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