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http://inaoe.repositorioinstitucional.mx/jspui/handle/1009/312| Modeling the infrared excess of solar analogs | |
| FERNANDO CRUZ SAENZ DE MIERA | |
| MIGUEL Y ROSA MARIA CHAVEZ DAGOSTINO OLGA MERCEDES VEGA CASANOVA EMANUELE BERTONE TARICCO | |
| Acceso Abierto | |
| Atribución-NoComercial-SinDerivadas | |
| Modeling Circumstellar matter Infrared sources Solar analogs | |
| During 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. | |
| Instituto Nacional de Astrofísica, Óptica y Electrónica | |
| 2012-02 | |
| Tesis de maestría | |
| Inglés | |
| Estudiantes Investigadores Público en general | |
| Cruz-Sáenz-de-Miera F. | |
| ASTRONOMÍA Y ASTROFÍSICA | |
| Versión aceptada | |
| acceptedVersion - Versión aceptada | |
| Aparece en las colecciones: | Maestría en Astrofísica |
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| Fichero | Descripción | Tamaño | Formato | |
|---|---|---|---|---|
| SaenzMFC.pdf | 9.01 MB | Adobe PDF | Visualizar/Abrir |