ISO Observations of the Infrared Continuum of the Herbig Ae/Be Stars

Details ISO Observations of the Infrared Continuum of the Herbig Ae/Be Stars ISO Observations of the Infrared Continuum of the Herbig Ae/Be Stars

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003cokon.103..109e&link_type=abstract

Communications of the Konkoly Observatory, Hungary Proceedings of the conference: 'The interaction of stars with their environme

Computer Science

Scientific paper

We present a study of the whole sample of the Herbig Ae/Be stars observed with the spectrometers on board of the Infrared Space Observatory (ISO/ESA). These objects have been studied not only by means of their infrared continuum emission but also with respect to all the available photometric data, collected from the optical region to the radio wavelengths. The global spectral energy distributions (SEDs) have been compared with the results of radiative transfer calculations, that have been made in the framework of a circumstellar (CS) model. The results of the selection of the best models allow us to infer on the relationship between the geometry of the CS matter distribution and the evolutionary stage of these objects.

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