The Initial Mass Function of Be Stars
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Published:2004
Issue:
Volume:215
Page:83-84
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ISSN:0074-1809
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Container-title:Symposium - International Astronomical Union
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language:en
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Short-container-title:Symp. - Int. Astron. Union
Author:
Zorec J.,Levenhagen R.,Chauville J.,Frémat Y.,Ballereau D.,Hubert A. M.,Floquet M.,Leister N. V.
Abstract
Allowing for systematic differences in the counting of Be Stars due to their overluminosity, changes produced by their fast rotation on spectral types and time spent in the main sequence, a difference between the IMF (Be) and IMF(B) appears, which indicates that the appearance of the Be phenomenon may relay on differences in the initial star formation conditions.
Publisher
Cambridge University Press (CUP)