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A new B-subdwarf eclipsing binary with an extremely short period
Published online by Cambridge University Press: 04 August 2017
Abstract
The B-type Subdwarf BD-07°3477 has been found to be an eclipsing binary with a period of about 2h48m. A preliminary analysis of the light curve reveals the system to be fully detached. It appears to be similar in many respects to the O-Subdwarf binary AA Dor which is thought to be the remnant of a system which has undergone a common envelope phase of evolution.
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- II. Photometric Research Programmes
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- Copyright © Reidel 1986
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