Progress on the photometric study of short-period eclipsing binaries

dc.creatorGomez, M.
dc.creatorLapasset, E.
dc.creatorAhumada, J.
dc.creatorClariá, J.J.
dc.creatorMinniti, D.
dc.date1988
dc.date2022-09-13T14:38:19Z
dc.date.accessioned2023-07-15T08:05:04Z
dc.date.available2023-07-15T08:05:04Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/142001
dc.identifierissn:1669-9521
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7482966
dc.descriptionPartial light curves and updated ephemeris of seven short-period eclipsing binaries: V676 Centauri, HY Pavonis, AA Ceti, BP Velorum, RT Hydri, BF Pavonis and BC Gruis are presented. The photometric UBV observations were obtained with the 76 cm telescope at El Leóncito (Félix Aguilar Station) and with the 2.15 m telescope at CASLEO Observatory. The period of BC Gru was substantially modified. All the observed systems present the typical characteristics of close binaries with different degrees of thermal contact.
dc.descriptionAsociación Argentina de Astronomía
dc.formatapplication/pdf
dc.languagees
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.subjectAstronomía
dc.subjectGalaxia
dc.subjectv676 Cen
dc.subjecthy pav
dc.subjectaa cet
dc.subjectbp vel
dc.subjectr hya
dc.subjectbf pav
dc.subjectbc gru
dc.titleProgress on the photometric study of short-period eclipsing binaries
dc.typeArticulo
dc.typeComunicacion


Este ítem pertenece a la siguiente institución