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Measurements of Masses and Radii of Eclipsing Binaries

Published online by Cambridge University Press:  12 April 2016

S. Ferluga ,
L. Floreano  and
D. Mangiacapra
S. Ferluga
Affiliation:
Dipartimento di Astronomia, Università di Trieste Via G.B. Tiepolo, 11 - I 34131 Trieste, Italy
L. Floreano
Affiliation:
Dipartimento di Astronomia, Università di Trieste Via G.B. Tiepolo, 11 - I 34131 Trieste, Italy
D. Mangiacapra
Affiliation:
Dipartimento di Astronomia, Università di Trieste Via G.B. Tiepolo, 11 - I 34131 Trieste, Italy

Abstract

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We report the detection of 10 new double–line eclipsing binary systems, with first measurements of masses and radii. These results are the preliminary outcome of an observational campaign for detecting new double–line eclipsing systems, carried out at the Observatoire de Haute Provence (OHP) in France, with the 1.52-m telescope and its CCD high–resolution spectrograph Aurelie.

Type
IV. Input physics and basic stellar data
Information
International Astronomical Union Colloquium , Volume 137: Inside the Stars , 1993 , pp. 364 - 367
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

Batten, A.H., Fletcher, J.M., Mac Carthy, D.G.: 1989, Eighth Catalogue of the Orbital Elements of spectroscopic Binary Systems, Publ. Dominion Astroph. Observatory (Victoria, Canada) 17, 1 Google Scholar
Cester, B., Fedel, B., Giuricin, G., Mardirossian, F., Mezzetti, M., Predolin, F.: 1979, A Catalogue of modern Lightcurve Synthesis photometric Solutions of close Binary Systems, Mem. Soc. Astron. Italiana 50, 553 Google Scholar
Ferluga, S., Floreano, L., Mangiacapra, D.: 1991, La Lettre de l’OHP (Publ. Obs. Haute Provence, France) 6, 3 Google Scholar