On the Be and Ae Stars in NGC 6611

The young cluster NGC 6611 is of interest because it has been believed to contain an unusually large number of Be and Ae stars. The cluster is embedded in a very bright Hiiregion, so that proper subtraction of that background on slit or multiobject fiber‐fed spectra is important. If stellar line emi...

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Bibliographic Details
Published inPublications of the Astronomical Society of the Pacific Vol. 113; no. 780; pp. 195 - 196
Main Authors Herbig, G. H., Dahm, Scott E.
Format Journal Article
LanguageEnglish
Published The University of Chicago Press 01.02.2001
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