Barbosa |
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Bastian |
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Blum |
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Brott |
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Caballero |
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Chen |
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Chita |
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Chu |
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Churchwell |
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Corcoran |
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Crowther |
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Damineli et al |
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Damineli |
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Fullerton |
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Gagne |
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Gallagher |
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Garcia |
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Garmany |
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Georgiev |
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Hamann |
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Hillier |
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Howarth |
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Indebetouw |
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Kobulnicky |
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Koenigsberger |
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Lang |
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Leitherer |
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Lennon |
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Levesque |
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Linder |
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Maeder |
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Mahy |
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Massa |
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Massey |
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McSwain |
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Moffat |
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Moises |
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Morrell |
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Morris |
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Naze |
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Nieva |
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Olsen |
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Oskinova |
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Owocki |
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Penny |
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Przybilla |
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Skinner |
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Smith |
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Soderberg |
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Teodoro |
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Testor |
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Townsley |
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Vacca |
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Vink |
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Wachter |
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Walborn |
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Wallerstein |
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Whelan |
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Williams |
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Willis |
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Wing |
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Wolff |
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van den Heuvel |
Spectral Synthesis of Massive Stars
Claus Leitherer
STScI
I will discuss recent developments in modeling the spectral energy distributions of massive stars. Special emphasis will be on the impact of new stellar evolution models with rotation. These new models can profoundly change the theoretically predicted spectra, in particular when hot stars are important. While some long-standing unresolved issues of spectral modeling are disappearing with these models, I will point out areas requiring future improvements.