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dc.date.accessioned 2022-12-07T15:18:40Z
dc.date.available 2022-12-07T15:18:40Z
dc.date.issued 1989
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/147001
dc.description.abstract The emission-line Of-, WR- and Be-type stars as members of open clusters are analyzed in particular related to their photometric data. It is found that amont the high-luminosity objects, the Of stars are the more common stars among the brightest members of open clusters. About 10% to 30% of the WR stars are members of open clusters. Those clusters with Of stars have much brighter apparent magnitude stars than those with WR-type stars. Concerning the Be stars, mostly are situated away of the main sequence; their color excesses E(B-V) of the circumstellar envelope is up to 0.3 magnitudes in extreme cases. en
dc.language es es
dc.subject Galaxia es
dc.title Astronomy in the catacombs: stars with special peculiarities as members of open clusters en
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Feinstein, Alejandro es
sedici.subject.materias Astronomía es
sedici.description.fulltext true es
mods.originInfo.place Asociación Argentina de Astronomía es
sedici.subtype Comunicacion es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.relation.journalTitle Boletín de la Asociación Argentina de Astronomía es
sedici.relation.journalVolumeAndIssue no. 35 es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)