6533b7d9fe1ef96bd126ce68

RESEARCH PRODUCT

Abundances of Be Stars in Very Young Open Clusters

Amparo MarcoJose M. TorrejonGuillermo BernabeuJ. J. RodesJuan Fabregat

subject

PhysicsPhotometryPhotometry (astronomy)StarsStar clusterBe starsFísica AplicadaAstronomyYoung open clustersBlue stragglerGalaxy clusterOpen clusterAstronomía y Astrofísica

description

The Be Phenomenon in Early-Type Stars, IAU Colloquium 175, ASP Conference Proceedings, Vol. 214, edited by Myron A. Smith and Huib F. Henrichs. Astronomical Society of the Pacific, ISBN 1-58381-045-5, 2000, p.59 We present here standard uvbyβ CCD photometry for five open clusters of the Galaxy in order to determine abundances of Be stars, as a function of age.

10.1017/s0252921100055597https://hdl.handle.net/10045/109359