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Eclipsing Binaries in Open Clusters

Published online by Cambridge University Press:  09 August 2007

John Southworth
John Southworth*
Affiliation:
Department of Physics, University of Warwick, Coventry, CV4 7AL, UK email: jkt@astro.keele.ac.uk
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Abstract

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Detached eclipsing binaries are very useful objects for calibrating theoretical stellar models and checking their predictions. Detached eclipsing binaries in open clusters are particularly important because of the additional constraints on their age and chemical composition from their membership of the cluster. I compile a list containing absolute parameters of well-studied eclipsing binaries in open clusters, and present new observational data on the B-type systems V1481 Cyg and V2263 Cyg which are members of the young open cluster NGC 7128.

Keywords

stars: binaries: eclipsingstars: binaries: closestars: distancesstars: evolutionstars: abundancesopen clusters and associations: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S240: Binary Stars as Critical Tools & Tests in Contemporary Astrophysics , August 2006 , pp. 619 - 621
Copyright
Copyright © International Astronomical Union 2007

References

Alencar, S. H. P., Vaz, L. P. R., Helt, B. E., 1997, A&A, 326, 709 Google Scholar
Andersen, J., Clausen, J. V., Nordström, B., 1990, ApJ, 363, L33 CrossRefGoogle Scholar
Bouzid, M. Y., Sterken, C., Pribulla, T., 2005, A&A, 437, 769 Google Scholar
Bragaglia, A., Tosi, M., 2006, AJ, 131, 1544 CrossRefGoogle Scholar
Chaboyer, B., 1995, ApJ, 444, L9 CrossRefGoogle Scholar
Claret, A., Willems, B., 2002, A&A, 388, 518 Google Scholar
Debernardi, Y., North, P., 2001, A&A, 374, 204 Google Scholar
Eldridge, J. J., Tout, C. A., 2004, MNRAS, 353, 87 CrossRefGoogle Scholar
Hensberge, H., Pavlovski, K., Verschueren, W., 2000, A&A, 358, 553 Google Scholar
Lebreton, Y., Fernandes, J., Lejeune, T., 2001, A&A, 374, 540 Google Scholar
Ludwig, H.-G., Salaris, M., 1999, in ASP Conf. Ser. 173, p. 229CrossRefGoogle Scholar
Maeder, A., Meynet, G., 1989, A&A, 210, 155 Google Scholar
Meynet, G., Maeder, A., Ekström, S., 2005, in ASP Conf. Ser. 332, p. 228Google Scholar
Nordström, B., et al. 2004, A&A, 418, 989 Google Scholar
Pols, O. R., Tout, C. A., Schroder, K.-P., Eggleton, P. P., Manners, J., 1997, MNRAS, 289, 869 CrossRefGoogle Scholar
Ribas, I., Jordi, C., Giménez, Á., 2000, MNRAS, 318, L55 CrossRefGoogle Scholar
Southworth, J., Clausen, J. V., 2006a, A&A, acceptedGoogle Scholar
Southworth, J., Clausen, J. V., 2006b, Ap&SS, in pressGoogle Scholar
Southworth, J., Maxted, P. F. L., Smalley, B., 2004a, MNRAS, 349, 547 CrossRefGoogle Scholar
Southworth, J., Maxted, P. F. L., Smalley, B., 2004b, MNRAS, 351, 1277 CrossRefGoogle Scholar
Southworth, J., Zucker, S., Maxted, P. F. L., Smalley, B., 2004c, MNRAS, 355, 986 CrossRefGoogle Scholar
Southworth, J., Maxted, P. F. L., Smalley, B., 2004d, in ASP Conf. Ser. 318, p. 218CrossRefGoogle Scholar
Southworth, J., Smalley, B., Maxted, P. F. L., Etzel, P. B., 2004e, in IAU Symp. 224, p. 548CrossRefGoogle Scholar
Southworth, J., Maxted, P. F. L., Smalley, B., 2005a, A&A, 429, 645 Google Scholar
Southworth, J., et al. 2005b, MNRAS, 363, 529 CrossRefGoogle Scholar
Southworth, J., Maxted, P. F. L., Smalley, B., 2005c, in IAU Colloq. 196, p. 361CrossRefGoogle Scholar
Thompson, I. B., et al. 2001, AJ, 121, 3089 CrossRefGoogle Scholar
Torres, G., Ribas, I., 2002, ApJ, 567, 1140 CrossRefGoogle Scholar
VandenBerg, D. A., Bergbusch, P. A., Dowler, P. D., 2006, ApJS, 162, 375 CrossRefGoogle Scholar