Pre-Main Sequence Stars Seen by ISO

Details Pre-Main Sequence Stars Seen by ISO Pre-Main Sequence Stars Seen by ISO

Aug 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ssrv..119..181l&link_type=abstract

Space Science Reviews, Volume 119, Issue 1-4, pp. 181-199

Physics

2

Pre-Main Sequence, Circumstellar Matter, Iso, Infrared Spectroscopy

Scientific paper

Observations of pre-main sequence objects (T Tauri, Herbig Ae/Be and FU Orionis stars) obtained with the instrumentation on board the Infrared Space Observatory (ISO) are reviewed. All the observations have been mainly carried out by using the two spectrographs SWS and LWS, adopting their low resolution modes and such data have been used both for lines detection and to reconstruct the spectral energy distributions. Line emission and photometric behaviour of pre-main sequence objects have been analyzed in the framework of the current models, discussing the agreement (or disagreement) with them and trying to derive the questions which should be answered by the forthcoming FIR instrumentation.

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