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dc.provenanceCONICET-
dc.creatorMiroshnichenko, A. S.-
dc.creatorManset, N.-
dc.creatorZharikov, S. V.-
dc.creatorZsargó, J.-
dc.creatorJuárez Jiménez, J. A.-
dc.creatorGroh, J. H.-
dc.creatorLevato, Orlando Hugo-
dc.creatorGrosso, Monica Gladys-
dc.creatorRudy, R. J.-
dc.creatorLaag, E. A.-
dc.creatorCrawford, K. B.-
dc.creatorPuetter, R. C.-
dc.creatorReichart, D. E.-
dc.creatorIvarsen, K. M.-
dc.creatorHaislip, J. B.-
dc.creatorNysewander, M. C.-
dc.creatorLaCluyze, A. P.-
dc.date2016-03-30T16:35:28Z-
dc.date2016-03-30T16:35:28Z-
dc.date2014-01-
dc.date2016-05-06 15:52:43.262787-03-
dc.date.accessioned2019-04-29T15:39:23Z-
dc.date.available2019-04-29T15:39:23Z-
dc.date.issued2014-01-
dc.identifierMiroshnichenko, A. S.; Manset, N.; Zharikov, S. V.; Zsargó, J.; Juárez Jiménez, J. A.; et al.; Confirmation of the Luminous Blue Variable Status of MWC 930; Hindawi Publishing Corporation; Advances in Astronomy; 2014; 1-2014; 1-9-
dc.identifier1687-7969-
dc.identifierhttp://hdl.handle.net/11336/4974-
dc.identifier.urihttp://rodna.bn.gov.ar:8080/jspui/handle/bnmm/298709-
dc.descriptionWe present spectroscopic and photometric observations of the emission-line star MWC 930 (V446 Sct) during its long-term optical brightening in 2006–2013. Based on our earlier data we suggested that the object has features found in Luminous Blue Variables (LBV), such as a high luminosity (∼3 105 L⊙), a low wind terminal velocity (∼140 km s−1), and a tendency to show strong brightness variations (∼1 mag over 20 years). For the last ∼7 years it has been exhibiting a continuous optical and near-IR brightening along with a change of the emission-line spectrum appearance and cooling of the star’s photosphere. We present the object’s -band light curve, analyze the spectral variations, and compare the observed properties with those of other recognized Galactic LBVs, such as AG Car and HR Car. Overall we conclude the MWC 930 is a bona fide Galactic LBV that is currently in the middle of an S Dor cycle-
dc.descriptionFil: Miroshnichenko, A. S.. University of North Carolina at Greensboro. Department of Physics and Astronomy; Estados Unidos-
dc.descriptionFil: Manset, N.. CFHT Corporation; Estados Unidos-
dc.descriptionFil: Zharikov, S. V.. Universidad Nacional Autónoma de México; México-
dc.descriptionFil: Zsargó, J.. Instituto Politécnico Nacional. Escuela Superior de Física y Matemáticas. Departamento de Fisica; México-
dc.descriptionFil: Juárez Jiménez, J. A.. Instituto Politécnico Nacional. Escuela Superior de Física y Matemáticas. Departamento de Fisica; México-
dc.descriptionFil: Groh, J. H.. Geneva University. Geneva Observatory; Suiza-
dc.descriptionFil: Levato, Orlando Hugo. Consejo Nacional de Investigaciones Cienti­ficas y Tecnicas. Centro Cientifico Tecnologico San Juan. Instituto de Ciencias Astronomicas de la Tierra y del Espacio; Argentina-
dc.descriptionFil: Grosso, Monica Gladys. Consejo Nacional de Investigaciones Cienti­ficas y Tecnicas. Centro Cientifico Tecnologico San Juan. Instituto de Ciencias Astronomicas de la Tierra y del Espacio; Argentina-
dc.descriptionFil: Rudy, R. J.. The Aerospace Corporation; Estados Unidos-
dc.descriptionFil: Laag, E. A.. The Aerospace Corporation; Estados Unidos-
dc.descriptionFil: Crawford, K. B.. The Aerospace Corporation; Estados Unidos-
dc.descriptionFil: Puetter, R. C.. University of California at San Diego. Center for Astrophysics and Space Science; Estados Unidos-
dc.descriptionFil: Reichart, D. E.. University of North Carolina. Department of Physics and Astronomy; Estados Unidos-
dc.descriptionFil: Ivarsen, K. M.. University of North Carolina. Department of Physics and Astronomy; Estados Unidos-
dc.descriptionFil: Haislip, J. B.. University of North Carolina. Department of Physics and Astronomy; Estados Unidos-
dc.descriptionFil: Nysewander, M. C.. University of North Carolina. Department of Physics and Astronomy; Estados Unidos-
dc.descriptionFil: LaCluyze, A. P.. University of North Carolina. Department of Physics and Astronomy; Estados Unidos-
dc.formatapplication/pdf-
dc.formatapplication/pdf-
dc.languageeng-
dc.publisherHindawi Publishing Corporation-
dc.relationinfo:eu-repo/semantics/altIdentifier/url/http://www.hindawi.com/journals/aa/2014/130378/abs/-
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1155/2014/130378-
dc.rightsinfo:eu-repo/semantics/openAccess-
dc.rightshttps://creativecommons.org/licenses/by/2.5/ar/-
dc.sourcereponame:CONICET Digital (CONICET)-
dc.sourceinstname:Consejo Nacional de Investigaciones Científicas y Técnicas-
dc.sourceinstacron:CONICET-
dc.source.urihttp://hdl.handle.net/11336/4974-
dc.subjectStars-
dc.subjectB[e] stars-
dc.subjectLuminous stars-
dc.subjectAstronomía-
dc.subjectCiencias Físicas-
dc.subjectCIENCIAS NATURALES Y EXACTAS-
dc.titleConfirmation of the Luminous Blue Variable Status of MWC 930-
dc.typeinfo:eu-repo/semantics/article-
dc.typeinfo:eu-repo/semantics/publishedVersion-
dc.typeinfo:ar-repo/semantics/articulo-
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