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

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

Jul 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..272..620m&link_type=abstract

Active OB stars: structure, evolution, mass loss, and critical limits, Proceedings of the International Astronomical Union, IAU

Astronomy and Astrophysics

Astronomy

1

Stars: Emission-Line, Be, Circumstellar Matter, Stars: Fundamental Parameters

Scientific paper

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.

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