Star formation and early evolution in the ISO data-base

Details Star formation and early evolution in the ISO data-base Star formation and early evolution in the ISO data-base

Feb 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.511..111n&link_type=abstract

Exploiting the ISO Data Archive. Infrared Astronomy in the Internet Age, held in Siguenza, Spain 24-27 June, 2002. Edited by

Astronomy and Astrophysics

Astronomy

Scientific paper

In this contribution, I will summarize the observations available in the ISO Data Archive concerning the different phases of the star formation process, focusing in particular on the low mass young stars. I will also address possible projects on specific issues of the young star evolution which remain still uncovered. As an example of a large project exploiting the ISO Data Archive I will finally show the results of a far infrared spectroscopic survey performed on a sample of 54 Young Stellar Objects (YSOs) in different evolutionary phases, from the youngest protostars to pre-main sequence stars. Such a study has allowed to define average spectroscopical properties of different classes of YSOs, which will be useful for the definition of programmes for future space missions.

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