The Be star content of young open clusters

Details The Be star content of young open clusters The Be star content of young open clusters

2002-10-30

arxiv.org/abs/astro-ph/0210653v1

Astronomy and Astrophysics

Astrophysics

6 pages, to be published in ASP Conference Series "Interplay between periodic, cyclic and stochastic variability in selected a

Scientific paper

We present a photometric survey aimed to characterize the Be star population
of young open clusters. It is found that in these clusters early-type Be stars
are more frequent than in the galactic field, and late-type Be stars are scarce
or inexistent. We interpret this result as evidence for an evolutionary
enhancement of the Be phenomenon towards the end of the main sequence lifetime.

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