Spectral synthesis for Be stars

A new monochromatic imaging and spectral synthesis package for Be stars, based on the bedisk code, is introduced. Example images and spectra are given for for H i and Fe ii. Predicted Fe ii equivalents widths are also compared to recent observations by Arias et al. (2006) and show good agreement, al...

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Bibliographic Details
Published inProceedings of the International Astronomical Union Vol. 6; no. S272; pp. 426 - 427
Main Author Sigut, T. A. Aaron
Format Journal Article
LanguageEnglish
Published Cambridge, UK Cambridge University Press 01.07.2010
Subjects
Accretion disks
Astrophysics
Contributed Papers
Spectrum analysis
Stars & galaxies
Be
stars: emission-line
circumstellar matter
radiative transfer
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Summary:A new monochromatic imaging and spectral synthesis package for Be stars, based on the bedisk code, is introduced. Example images and spectra are given for for H i and Fe ii. Predicted Fe ii equivalents widths are also compared to recent observations by Arias et al. (2006) and show good agreement, although only for very dense disks.
Bibliography:ObjectType-Article-1
SourceType-Scholarly Journals-1
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ISSN:1743-9213
1743-9221
DOI:10.1017/S1743921311011045