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Determination of fundamental parameters and circumstellar properties for a sample of B[e] stars

Published online by Cambridge University Press:  12 July 2011

María F. Muratore ,
Lydia S. Cidale ,
María L. Arias ,
Juan Zorec  and
Andrea F. Torres
María F. Muratore
Affiliation:
Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata, Paseo del Bosque S/N, 1900 La Plata, Argentina email: fmuratore@carina.fcaglp.unlp.edu.ar
Lydia S. Cidale
Affiliation:
Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata, Paseo del Bosque S/N, 1900 La Plata, Argentina email: fmuratore@carina.fcaglp.unlp.edu.ar Instituto de Astrofísica La Plata, CCT La Plata, CONICET, Paseo del Bosque S/N, 1900 La Plata, Argentina
María L. Arias
Affiliation:
Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata, Paseo del Bosque S/N, 1900 La Plata, Argentina email: fmuratore@carina.fcaglp.unlp.edu.ar Instituto de Astrofísica La Plata, CCT La Plata, CONICET, Paseo del Bosque S/N, 1900 La Plata, Argentina
Juan Zorec
Affiliation:
Institut d'Astrophysique de Paris, UPMC, UMR7095 CNRS, Paris, France
Andrea F. Torres
Affiliation:
Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata, Paseo del Bosque S/N, 1900 La Plata, Argentina email: fmuratore@carina.fcaglp.unlp.edu.ar Instituto de Astrofísica La Plata, CCT La Plata, CONICET, Paseo del Bosque S/N, 1900 La Plata, Argentina
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Abstract

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We develop a simple model to derive theoretical continuum energy distributions for B[e] stars, consisting of a B star surrounded by an envelope made of gas and dust. We select a sample of B[e] objects for which we construct the observed energy distributions, from 0.1 to 100 μm, using available photometric and spectroscopic data. We present some preliminary fittings.

Keywords

stars: emission-lineBecircumstellar matterstars: fundamental parameters
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S272: Active OB stars: structure, evolution, mass loss, and critical limits , July 2010 , pp. 620 - 621
Copyright
Copyright © International Astronomical Union 2011

References

Cardelli, J. A., Clayton, G. C., & Mathis, J. S. 1989, ApJ, 345, 245Google Scholar
Cidale, L. S. & Ringuelet, A. E. 1989, PASP, 101, 417CrossRefGoogle Scholar
Lamers, H. J. G. L. M., Zickgraf, F.-J., de Winter, D., Houziaux, L. et al. 1998, A&A, 340, 117Google Scholar
Moujtahid, A. 1998, Thèse de Doctorat, Université Paris VIGoogle Scholar
Moujtahid, A., Zorec, J., & Hubert, A. M. 1999, A&A, 349, 151Google Scholar