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Synthetic high-resolution line spectra of star-forming galaxies below 1200 Å, based on FUSE spectral libraries of hot stars

Published online by Cambridge University Press:  26 May 2016

Carmelle Robert ,
Anne Pellerin ,
Alessandra Aloisi ,
Claus Leitherer ,
Charles G. Hoopes  and
Timothy M. Heckman
Carmelle Robert
Affiliation:
Département de physique, Université Laval and Observatoire du mont Mégantic, Québec, QC, G1K 7P4, Canada
Anne Pellerin
Affiliation:
Département de physique, Université Laval and Observatoire du mont Mégantic, Québec, QC, G1K 7P4, Canada
Alessandra Aloisi
Affiliation:
Department of Physics and Astronomy, The Johns Hopkins University, 3400 North Charles Street, Baltimore, MD 21218, USA
Claus Leitherer
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA
Charles G. Hoopes
Affiliation:
Department of Physics and Astronomy, The Johns Hopkins University, 3400 North Charles Street, Baltimore, MD 21218, USA
Timothy M. Heckman
Affiliation:
Department of Physics and Astronomy, The Johns Hopkins University, 3400 North Charles Street, Baltimore, MD 21218, USA

Abstract

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We have generated far-UV stellar libraries using spectra of hot stars in the Galaxy and the Large and Small Magellanic Clouds. These libraries were implemented into the stellar population synthesis codes starburst99 and lavalsb and used to compute synthetic spectra of star-forming galaxies. Model spectra for galaxies are presented and variations of the hot star photospheric and wind profiles are discussed. This poster summarizes the work of Robert et al. (2002).

Type
Part 4. Feedback from Massive Stars
Information
Symposium - International Astronomical Union , Volume 212: A Massive Star Odyssey: From Main Sequence to Supernova , 2003 , pp. 744 - 746
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

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