Photometric and spectroscopic variations of the Be star HD 112999

dc.creatorWeidmann, Walter Alfredo
dc.creatorGamen, Roberto Claudio
dc.creatorAidelman, Yael Judith
dc.creatorFerrero, G. A.
dc.creatorCorti, Mariela Alejandra
dc.date.accessioned2016-09-07T19:18:09Z
dc.date.accessioned2018-11-06T16:11:18Z
dc.date.available2016-09-07T19:18:09Z
dc.date.available2018-11-06T16:11:18Z
dc.date.created2016-09-07T19:18:09Z
dc.date.issued2013-06
dc.identifierWeidmann, Walter Alfredo; Gamen, Roberto Claudio; Aidelman, Yael Judith; Ferrero, G. A.; Corti, Mariela Alejandra; Photometric and spectroscopic variations of the Be star HD 112999; Konkoly Observatory; Information Bulletin on Variable Stars; 6060; 6-2013; 1-8
dc.identifier0374-0676
dc.identifierhttp://hdl.handle.net/11336/7522
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1905378
dc.description.abstractBe objects are stars of B spectral type showing lines of the Balmer series in emission. The presence of these lines is attributed to the existence of an extended envelope, disk type, around them. Some stars are observed in both the Be and normal B-type spectroscopic states and they are known as transient Be stars. In this paper we show the analysis carried out on a new possible transient Be star, labelled HD 112999, using spectroscopic optical observations and photometric data.
dc.languageeng
dc.publisherKonkoly Observatory
dc.relationinfo:eu-repo/semantics/altIdentifier/url/http://ibvs.konkoly.hu/cgi-bin/IBVS?6060
dc.relationinfo:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1305.7098v1
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.rightsinfo:eu-repo/semantics/openAccess
dc.subjectSTARS: EMISSION-LINE
dc.subjectSTARS:Be
dc.subjectSTARS: INDIVIDUAL: HD 112999
dc.subjectSTARS: VARIABLES: GENERAL
dc.titlePhotometric and spectroscopic variations of the Be star HD 112999
dc.typeArtículos de revistas
dc.typeArtículos de revistas
dc.typeArtículos de revistas


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