Features of Sources of Radiation in the Environment of Young Stars

Details Features of Sources of Radiation in the Environment of Young Stars Features of Sources of Radiation in the Environment of Young Stars

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010vsgh.conf..193i&link_type=abstract

Variable Stars, the Galactic halo and Galaxy Formation, Proceedings of an international conference held in Zvenigorod, Russia, 1

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Using the results of broad-band ground-based and extra-atmospheric infrared photometric observations, we studied the spectral energy distributions of 87 young stars in the 0.36-100 μm range. Only 5 types of SED curves are met among the objects of our sample. We suggest to append the photometric classification scheme based on the IR spectra of young stars, earlier introduced by other authors. For some stars, we observe up to three wavelength intervals with excess radiation in the spectrum, which can be explained with the presence of additional thermal radiation sources in the system. The most probable temperatures of these sources are {˜}1500{-}2500 and 90{-}120 K.

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