Far Infrared Spectroscopy of Pre-Main Sequence Stars: The Lesson Learned from ISO and Perspectives

Details Far Infrared Spectroscopy of Pre-Main Sequence Stars: The Lesson Learned from ISO and Perspectives Far Infrared Spectroscopy of Pre-Main Sequence Stars: The Lesson Learned from ISO and Perspectives

Jul 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001esasp.460..451l&link_type=abstract

The Promise of the Herschel Space Observatory. Eds. G.L. Pilbratt, J. Cernicharo, A.M. Heras, T. Prusti, & R. Harris. ESA-SP 460

Physics

Stars: Circumstellar Matter, Stars: Formation, Infrared: Ism: Lines, Infrared: Stars

Scientific paper

We have recently analyzed the ISO-LWS spectra (43-197 microns) of two classes of Pre-Main Sequence objects, the Herbig Ae/Be (HAEBE) and the FU Orionis stars. ISO-LWS has provided an unbiased view of the neighbourhood of the central object by sampling the physical scale (≈ 80 arcsec) where the interaction with the closeby environment is taking place. The obtained spectroscopical results along with the comparison with model predictions are reviewed here. However, these far IR surveys have pointed out how remarkable aspects remain still unaddressed and have originated new questions which can be answered by using the capabilities offered by FIRST.

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