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Quantitative Spectroscopy of Close Binary Stars

2012
The method of spectral disentangling has now created the opportunity for studying the chemical composition in previously inaccessible components of binary and multiple stars. This in turn makes it possible to trace their chemical evolution, a vital aspect in understanding the evolution of stellar systems.
openaire  

Presupernova Evolution of Massive Single and Binary Stars

Annual Review of Astronomy and Astrophysics, 2012
Norbert Langer
exaly  

A search for close binary systems in the SALT survey of hydrogen-deficient stars using TESS

Monthly Notices of the Royal Astronomical Society
Edward Snowdon   +2 more
exaly  

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