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A new B-subdwarf eclipsing binary with an extremely short period

Published online by Cambridge University Press:  04 August 2017

J W Menzies and
F Marang
J W Menzies
Affiliation:
South African Astronomical Observatory P O Box 9 Observatory 7935 South Africa
F Marang
Affiliation:
South African Astronomical Observatory P O Box 9 Observatory 7935 South Africa

Abstract

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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.

Information

Type
II. Photometric Research Programmes
Information
Symposium - International Astronomical Union , Volume 118: Instrumentation and Research Programmes for Small Telescopes , 1986, pp. 305 - 306
Copyright
Copyright © Reidel 1986 

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