Free Access
Issue |
A&A
Volume 452, Number 3, June IV 2006
|
|
---|---|---|
Page(s) | 959 - 967 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361:20053270 | |
Published online | 06 June 2006 |
- Berthold, T. 1981, Inf. Bull. Var. Stars No. 1942 [Google Scholar]
- Berthold, T. 1983, Inf. Bull. Var. Stars No. 2443 [Google Scholar]
- Cereda, L., Mist, A., Niarchos, P. G., & Poretti, E. 1988, A&AS, 76, 255 [NASA ADS] [Google Scholar]
- Davidge, T. J., & Milone, E. F. 1984, ApJS, 55, 571 [NASA ADS] [CrossRef] [Google Scholar]
- Diethelm, R. 1981, BBSAG No. 52, 71 [Google Scholar]
- Donato, L., Lepardo, A., Santini, V., et al. 2003, Inf. Bull. Var. Stars No. 5391 [Google Scholar]
- Duerbeck, H. W. 1984, Mitt. Astr. Gesell., 62, 87 [NASA ADS] [Google Scholar]
- Flannery, B. P. 1976, ApJ, 205, 217 [Google Scholar]
- Harris, A. W. 1979, Inf. Bull. Var. Stars No. 1556 [Google Scholar]
- Harris, A. W. 1982, IAPPP Comm No, 10, 44 [Google Scholar]
- Kallrath, J., & Milone, E. F. 1999, Eclipsing Binaries - Modeling and Analysis (New York: Springer) [Google Scholar]
- Kallrath, J., Milone, E. F., Terrell, D., & Young, A. T. 1998, ApJS, 508, 308 [NASA ADS] [CrossRef] [Google Scholar]
- Kurucz, R. L. 1979, ApJS, 40, 1 [NASA ADS] [CrossRef] [Google Scholar]
- Kurucz, R. L. 1993, in Light Curve Modeling of Eclipsing Bianary Stars, ed. E. F. Milone (New York: Springer), 93 [Google Scholar]
- Kwee, K. K., & van Woerden, H. 1956, Bull. Astron. Inst. Neth., 12, 327 [NASA ADS] [Google Scholar]
- Linnell, A. P., & Proctor, D. D. 1970, ApJ, 162, 683 [NASA ADS] [CrossRef] [Google Scholar]
- Liu, Q., & Yang, Y. 2000, A&AS, 142, 31 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
- Lu, W. 1993, AJ, 105, 646 [NASA ADS] [CrossRef] [Google Scholar]
- Lucy, L. B. 1967, ZfAp, 65, 89 [Google Scholar]
- Maceroni, C., & Van't Veer, F. 1996, A&A, 311, 523 [NASA ADS] [Google Scholar]
- Milone, E. F. 2003, in GAIA Spectroscopy, Science and Technology, ed. U. Munari, ASP Conf. Ser., 298, 303 [NASA ADS] [Google Scholar]
- Milone, E. F., Wilson, R. E., & Hrivnak, B. J. 1987, ApJ, 318, 325 M [Google Scholar]
- Mochnacki, S. W. 1985, in Interacting Binaries, ed. P. P. Eggleton [Google Scholar]
- Munari, U., Tomov, T., Zwitter, T., et al. 2001, A&A, 378, 477 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
- Paresce, F. 1984, AJ, 89, 1022 [NASA ADS] [CrossRef] [Google Scholar]
- Qian, S. 2001, MNRAS, 328, 635 [NASA ADS] [CrossRef] [Google Scholar]
- Robertson, J. A., & Eggleton, P. P. 1977, MNRAS, 179, 359 [NASA ADS] [Google Scholar]
- Rucinski, S. M. 1974, Acta Astron., 24, 119 [NASA ADS] [Google Scholar]
- Rucinski, S. M. 1985, in Interacting Binary Stars, ed. J. E. Pringle, & R. A. Wade (Cambridge University Press), 113 [Google Scholar]
- Twigg, L. W., & Rafert, J. B. 1980, MNRAS, 193, 775 [NASA ADS] [CrossRef] [Google Scholar]
- Van Hamme, W. 1993, AJ, 106, 2096 [NASA ADS] [CrossRef] [Google Scholar]
- Van Hamme, W., Samec, R. G., Gothard, N. W., et al. 2001, AJ, 122, 3446 [Google Scholar]
- Wilson, R. E., & Devinney, E. J. 1971, ApJ, 166, 605 [NASA ADS] [CrossRef] [Google Scholar]
- Wilson, R. E. 1979, ApJ, 234, 1054 [NASA ADS] [CrossRef] [Google Scholar]
- Wilson, R. E. 1988, Physical models for close binaries and logical constraints, in Critical Observations Versus Physical Models for Close Binary Systems, ed. K.-C. Leung (Montreux, Switzerland: Gordon and Breach), 193 [Google Scholar]
- Wilson, R. E. 2005, Ap&SS, 299, 197-207 [NASA ADS] [CrossRef] [Google Scholar]
- Yakut, K., Ulas, B., Kalomeni, B., & Gülmen, Ö. 2005, MNRAS, 363, 1272 [NASA ADS] [CrossRef] [Google Scholar]
- Zwitter, T., Munari, U., Marrese, P. M., et al. 2003, A&A, 404, 333 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.