BCD spectrophotometry of stars with the B[e] phenomenon : I. Fundamental Parameters

Low resolution spectra in the λλ3500-4600 Å wavelength range of 23 stars with the B[e] phenomenon are presented. Spectral classification of 15 program stars was performed using the BCD spectrophotometric system, based on the study of the Balmer discontinuity, which is independent of interstellar and...

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Detalles Bibliográficos
Autores principales: Cidale, Lydia Sonia, Zorec, Juan, Tringaniello, María Luján Ramona
Formato: Articulo
Lenguaje:Inglés
Publicado: 2001
Materias:
Ciencias Astronómicas
Geofísica, astronomía y astrofísica
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/2082
http://www.aanda.org/index.php?option=com_article&access=standard&Itemid=129&url=/articles/aa/full/2001/10/aa10323/aa10323.html
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata

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