Spectrophotometry of emission-line stars in the magellanic clouds

The strong emission lines in the most luminous stars in the Magellanic Clouds indicate that these stars have such strong stellar winds that their photospheres are so masked that optical absorption lines do not provide an accurate measure of photospheric conditions. In the research funded by this gra...

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Bibliographische Detailangaben
1. Verfasser: Bohannan, Bruce
Format: Report
Sprache:eng
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