Hostname: page-component-586b7cd67f-t8hqh Total loading time: 0 Render date: 2024-11-26T06:59:38.879Z Has data issue: false hasContentIssue false
  • English
  • Français

Low-Mass Eclipsing Binaries to Refine Barnes-Evans–Like Relations

Published online by Cambridge University Press:  09 August 2007

Pedro J. Amado
Pedro J. Amado*
Affiliation:
Dpto. de Física Teórica y del Cosmos, Facultad de Ciencias, Universidad de Granada, Spain; Instituto de Astrofsica de Andalucía-CSIC, Granada, Spain email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The relation of the surface brightness, a parameter related to the apparent magnitude and the angular diameter of a star, with a colour index is used to determine various stellar parameters. Eclipsing spectroscopic binaries can even be used as a distance indicator. In this work, we use a number of low-mass eclipsing binaries, whose parameters have been accurately determined, to refine the Barnes-Evans–like relation FV − (Ic − K) introduced by Amado et al. (1999), a relation more suitable for the low temperature of these cool stars.

Keywords

binaries: eclipsingstars: fundamental parametersstars: late-typestars: low-mass
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. 634 - 637
Copyright
Copyright © International Astronomical Union 2007

References

Allen, C.W. 1973, Astrophysical Quantities, Athone Press, London Google Scholar
Amado, P.J., Butler, C.J., & Byrne, P.B. 1999, MNRAS, 310, 1023 CrossRefGoogle Scholar
Barnes, T.G. & Evans, D.S. 1976, MNRAS, 174, 489 CrossRefGoogle Scholar
Barnes, T.G., Evans, D.S., & Moffett, T.J. 1978, MNRAS, 183, 285 CrossRefGoogle Scholar
Bell, R.A. & Gustafsson, B. 1980, MNRAS, 191, 435 CrossRefGoogle Scholar
Beuermann, K., Baraffe, I., & Hauschildt, P. 1999, A&A, 348, 524 Google Scholar
Creevey, O.L., Benedict, G.F., Brown, T.M., Alonso, R., Cargile, P., Mandushev, G., Charbonneau, D., McArthur, B.E., Cochran, W., O'Donovan, F.T., Jiménez-Reyes, S.J., Belmonte, J.A., & Kolinski, D. 2005, ApJ, 625, L127 CrossRefGoogle Scholar
Dawson, P.C. & De Robertis, M.M. 2004, AJ, 127, 2909 CrossRefGoogle Scholar
Leggett, S.K., Allard, F., Berriman, G., Dahn, C.C., & Hauschildt, P.H. 1996, ApJS, 104, 117 CrossRefGoogle Scholar
López-Morales, M. & Ribas, I. 2005, ApJ, 631, 1120 CrossRefGoogle Scholar
Maceroni, C. & Montalbán, J. 2004, A&A, 426, 577 Google Scholar
Moon, T.T. 1984, MNRAS, 211, 21 CrossRefGoogle Scholar
Ribas, I. 2003, A&A, 398, 239 Google Scholar
Torres, G. & Ribas, I. 2002, ApJ, 567, 1140 CrossRefGoogle Scholar
Viti, S., Jones, H. R.A., Schweitzer, A., Allard, F., Hauschildt, P.H., Tennyson, J., Miller, S., & Longmore, A.J. 1997, MNRAS, 291, 780 CrossRefGoogle Scholar
Wesselink, A.J. 1969, MNRAS, 144, 297 CrossRefGoogle Scholar
Young, T.B., Hidas, M.G., Webb, J.K., Ashley, M.C.B., Christiansen, J.L., Derekas, A., & Nutto, C. 2006, MNRAS, 370, 1529 CrossRefGoogle Scholar