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The Eclipsing Binary System LB3459

Published online by Cambridge University Press:  12 April 2016

D. Kilkenny ,
A.E. Lynas-Gray  and
R.W. Hilditch
D. Kilkenny
Affiliation:
University Observatory, St Andrews, Scotland
A.E. Lynas-Gray
Affiliation:
University Observatory, St Andrews, Scotland
R.W. Hilditch
Affiliation:
University Observatory, St Andrews, Scotland

Extract

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The extremely blue foreground LMC star LB3459 (= HDE 269696) was reported by Kilkenny, Hilditch and Penfold (1978) to be an eclipsing binary system with a period of 6h17m. Preliminary analysis of uvby photometry and data obtained with the University of Cape Town highspeed photometer (Nather 1973) indicated that the system was composed of two degenerate stars, probably 0-type subdwarfs.

Type
Colloquium Session IV
Information
International Astronomical Union Colloquium , Volume 53: White Dwarfs and Variable Degenerate Stars , August 1979 , pp. 255 - 258
Copyright
Copyright © The University of Rochester 1979

References

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