Autores
Dr.
Yakiv Pavlenko
Fecha y hora
16 Mayo 2013 - 10:30 Europe/London
Dirección
Aula
Idioma de la charla
Inglés
Número en la serie
1
Descripción
We discuss the role and significance of molecules in the modern astrophysics. Molecular opacities govern the structure of model atmospheres of late-type stars and ultracool dwarfs. Some problems of computations of model atmosphere and synthetical spectra of cool stars are discussed. We present some successful attempts of the application of the molecular spectroscpy for the studies of late -type stars and ultracool dwarfs. Finally, some problems of fitting theoretical spectra to the observed SED are discussed.