The Be star content of young open clusters
| dc.creator | Fabregat, Juan | |
| dc.date | 2002-10-30 | |
| dc.date.accessioned | 2026-07-07T02:05:54Z | |
| dc.date.available | 2026-07-07T02:05:54Z | |
| dc.description | 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. | |
| dc.description | 6 pages, to be published in ASP Conference Series "Interplay between periodic, cyclic and stochastic variability in selected areas of the H-R diagram", C. Sterken, Ed | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0210653 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0210653 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/5247 | |
| dc.subject | Astrophysics | |
| dc.title | The Be star content of young open clusters | |
| dc.type | text |