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Post Info TOPIC: V530 Orionis


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V530 Orionis
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Title: The Benchmark Eclipsing Binary V530 Ori: A Critical Test of Magnetic Evolution Models for Low-Mass Stars
Author: Guillermo Torres, Claud H. Sandberg Lacy, Kresimir Pavlovski, Gregory A. Feiden, Jeffrey A. Sabby, Hans Bruntt, Jens Viggo Clausen

We report accurate measurements of the physical properties (mass, radius, temperature) of components of the G+M eclipsing binary V530 Ori. The M-type secondary shows a larger radius and a cooler temperature than predicted by standard stellar evolution models, as has been found for many other low-mass stars and ascribed to the effects of magnetic activity and/or spots. We show that models from the Dartmouth series that incorporate magnetic fields are able to match the observations with plausible field strengths of 1-2 kG, consistent with a rough estimate we derive for that star.

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