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The PMS Eclipsing Binary RXJ 0529.4+0041

Published online by Cambridge University Press:  13 May 2016

E. Covino ,
S. Catalano ,
A. Frasca ,
E. Marilli ,
J.M. Alcalá ,
M. Fernández ,
C. Melo ,
R. Paladino  and
B. Stelzer
E. Covino
Affiliation:
1 Capodimonte Astronomical Observatory, Napoli, Italy
S. Catalano
Affiliation:
2 Catania Astrophysical Observatory, Italy
A. Frasca
Affiliation:
2 Catania Astrophysical Observatory, Italy
E. Marilli
Affiliation:
2 Catania Astrophysical Observatory, Italy
J.M. Alcalá
Affiliation:
1 Capodimonte Astronomical Observatory, Napoli, Italy
M. Fernández
Affiliation:
3 Max-Planck Institut für Extraterrestrische Physik, Garching, Germany
C. Melo
Affiliation:
4 Observatoire de Genève, Sauverny, Switzerland
R. Paladino
Affiliation:
1 Capodimonte Astronomical Observatory, Napoli, Italy
B. Stelzer
Affiliation:
3 Max-Planck Institut für Extraterrestrische Physik, Garching, Germany

Abstract

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We report the discovery of the first low–mass pre–main sequence eclipsing binary among a sample of double-lined spectroscopic binaries in the Orion star forming region found in a previous high-resolution spectroscopic investigation on ROSAT–discovered weak-T Tauri stars. Here we present the preliminary results from the combined analysis of the spectroscopic orbit and B and V light–curves, using data available till spring 2000. We then compare the fundamental stellar parameters derived from the orbital solution with those inferred from some widely used theoretical evolutionary models.

Type
XI. Young Binaries and Stellar Astrophysics
Information
Symposium - International Astronomical Union , Volume 200: The Formation of Binary Stars , 2001 , pp. 468 - 471
Copyright
Copyright © Astronomical Society of the Pacific 2001 

References

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