FUSE UV Spectral Energy Distributions of Pole-On Be Stars

Details FUSE UV Spectral Energy Distributions of Pole-On Be Stars FUSE UV Spectral Energy Distributions of Pole-On Be Stars

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001sf2a.conf...55f&link_type=abstract

Abstracts from SF2A-2001: Semaine de l'Astrophysique Francaise, meeting held in Lyon, France, May 28-June 1st, 2001, Eds.: F. Co

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Ultraviolet is a very important spectral range for the study of B type stars which radiates the biggest part of their energy between 900 and 2000 Å. Far UV spectra (905 - 1195 Å) have been obtained by FUSE for two pole-on Be stars and are decribed for the first time in our poster. Interstellar molecular bands and interstellar atomic lines are prevailing in this wavelength domain. Their presence strongly affects the stellar line profiles and lower significantly the star's (Photosphere + Envelope) energy distribution. We produce in the present work a computation of the effect of the interstellar medium on the Far UV spectra of the two studied stars (HD120991 & HD36408).

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