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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
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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2011

References

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