Massive Binaries in the Magellanic Clouds

Details Massive Binaries in the Magellanic Clouds Massive Binaries in the Magellanic Clouds

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005hia....13..463n&link_type=abstract

Highlights of Astronomy, Vol. 13, as presented at the XXVth General Assembly of the IAU - 2003 [Sydney, Australia, 13 - 26 July

Astronomy and Astrophysics

Astronomy

Scientific paper

We present results of our ongoing observing program on search and studies of massive stars (O and WR type) in binary systems in our neighbour galaxies the Magellanic Clouds. Radial velocity orbits are presented for new binaries and improved orbits for previously known systems. We compare orbital parameters of selected binaries containing O and WR type components. We also discuss the present status of knowledge for massive binary stars in the Magellanic Clouds and the problems encountered in their orbital studies such as stellar winds the ubiquitous tendency to be born in multiple systems etc..

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