B stars in open clusters: fundamental parameters

dc.creatorAidelman, Yael Judith
dc.creatorCidale, Lydia Sonia
dc.creatorZorec, Juan
dc.creatorArias, María Laura
dc.date2011-07-12
dc.date2019-10-25T14:26:12Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/84058
dc.identifierissn:1743-9213
dc.descriptionWe use the BCD spectrophotometric classification system to derive fundamental parameters of B stars in NGC 2439, NGC 3766 and NGC 6087. We are able to perform a complete study of each open cluster by deriving spectral classification of its members, distance modulus and age as well.
dc.descriptionFacultad de Ciencias Astronómicas y Geofísicas
dc.descriptionInstituto de Astrofísica de La Plata
dc.formatapplication/pdf
dc.format276-277
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.subjectCiencias Astronómicas
dc.subjectCiencias Exactas
dc.subjectBe
dc.subjectStars: distances
dc.subjectStars: emission-line
dc.subjectStars: fundamental parameters
dc.titleB stars in open clusters: fundamental parameters
dc.typeArticulo
dc.typeComunicacion


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