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

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 photo...

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Published inProceedings of the International Astronomical Union Vol. 6; no. S272; pp. 620 - 621
Main Authors Muratore, María F., Cidale, Lydia S., Arias, María L., Zorec, Juan, Torres, Andrea F.
Format Journal Article
LanguageEnglish
Published Cambridge, UK Cambridge University Press 01.07.2010
Subjects
Astrophysics
Contributed Papers
Matter & antimatter
Stars & galaxies
stars: fundamental parameters
Be
stars: emission-line
circumstellar matter
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Summary: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.
Bibliography:ObjectType-Article-1
SourceType-Scholarly Journals-1
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content type line 23
ISSN:1743-9213
1743-9221
DOI:10.1017/S1743921311011598