Modeling the infrared excess of solar analogs

dc.contributorMIGUEL Y ROSA MARIA CHAVEZ DAGOSTINO
dc.contributorOLGA MERCEDES VEGA CASANOVA
dc.contributorEMANUELE BERTONE TARICCO
dc.creatorFERNANDO CRUZ SAENZ DE MIERA
dc.date2012-02
dc.date.accessioned2023-07-25T16:21:19Z
dc.date.available2023-07-25T16:21:19Z
dc.identifierhttp://inaoe.repositorioinstitucional.mx/jspui/handle/1009/312
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7805532
dc.descriptionDuring the first months of the IRAS mission the science team attempted to conduct a series of calibration observations of α Lyrae (Vega), however, they unexpectedly found this star to be a copious IR source, with an emission at 60 and 100 μm far in excess to what was expected for a 10000 K blackbody, representing Vegas photosphere Aumann et al. [1984]. This indeed corresponds to one of the most important discoveries of the IRAS mission, perhaps, comparable with the also unexpected IR radiation detected from numerous early type galaxies which, until then, were considered devoid of significant amounts of interstellar matter.
dc.formatapplication/pdf
dc.languageeng
dc.publisherInstituto Nacional de Astrofísica, Óptica y Electrónica
dc.relationcitation:Cruz-Sáenz-de-Miera F.
dc.rightsinfo:eu-repo/semantics/openAccess
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/4.0
dc.subjectinfo:eu-repo/classification/Modelado/Modeling
dc.subjectinfo:eu-repo/classification/Materia circunstelar/Circumstellar matter
dc.subjectinfo:eu-repo/classification/Fuentes de infrarrojos/Infrared sources
dc.subjectinfo:eu-repo/classification/Analogos solares/Solar analogs
dc.subjectinfo:eu-repo/classification/cti/1
dc.subjectinfo:eu-repo/classification/cti/21
dc.subjectinfo:eu-repo/classification/cti/21
dc.titleModeling the infrared excess of solar analogs
dc.typeinfo:eu-repo/semantics/masterThesis
dc.typeinfo:eu-repo/semantics/acceptedVersion
dc.audiencestudents
dc.audienceresearchers
dc.audiencegeneralPublic


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