Tracing the young massive high-eccentricity binary system $\theta^{\mathsf 1}$Orionis C through periastron passage-Reference-Cited by-同舟云学术

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Tracing the young massive high-eccentricity binary system $\theta^{\mathsf 1}$Orionis C through periastron passage

Published:2009-02-09 Issue:1 Volume:497 Page:195-207
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Kraus S.,Weigelt G.,Balega Y. Y.,Docobo J. A.,Hofmann K.-H.,Preibisch T.,Schertl D.,Tamazian V. S.,Driebe T.,Ohnaka K.,Petrov R.,Schöller M.,Smith M.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361/200810368/pdf

Reference54 articles.

1. Physical conditions in the Orion Nebula and an assessment of its helium abundance

2. On the Accretion of Material by Theta Orionis C

3. Stellar mass-luminosity and mass-radius relations

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