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Pre-Main Sequence Stars Seen by ISO

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ISO Science Legacy

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Abstract

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 premain 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.

Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries: France, Germany, The Netherlands, and the United Kingdom), and with the participation of ISAS and NASA.

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Authors and Affiliations

  1. INAF, Osservatorio Astronomico di Roma, Via Frascati 33, 00040, Monte Porzio (Roma), Italy

    Dario Lorenzetti

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  1. Dario Lorenzetti
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Editors and Affiliations

  1. European Southern Observatory, Garching, Munich, Germany

    Catherine Cesarsky

  2. European Space Agency, Madrid, Spain

    Alberto Salama

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Lorenzetti, D. (2005). Pre-Main Sequence Stars Seen by ISO. In: Cesarsky, C., Salama, A. (eds) ISO Science Legacy. Springer, Dordrecht. https://doi.org/10.1007/1-4020-3844-5_8

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  • DOI: https://doi.org/10.1007/1-4020-3844-5_8

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  • Print ISBN: 978-1-4020-3843-3

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