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The Physical Conditions of Low Mass Star Forming Regions

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The Physics of Star Formation and Early Stellar Evolution

Part of the book series: NATO ASI Series ((ASIC,volume 342))

Abstract

The stellar population of dark molecular clouds and isolated Bok globules consist mainly of low mass stars. The physical conditions of these clouds from their largest to their smallest structures are reviewed and the different methods used to derive them are evaluated. The interaction of the newly born stars with the ambient gas is analyzed on the basis of new results obtained from high angular resolution molecular line observations.

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  1. IRAM, Av. Divina Pastora 7, NC, 18012, Granada, Spain

    J. Cernicharo

  2. Centro Astronómico de Yebes, Apartado 148, 19080, Guadalajara, Spain

    J. Cernicharo

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  1. Smithsonian Astrophysical Observatory, Cambridge, MA, USA

    Charles J. Lada

  2. Department of Physics, University of Crete, Heraklion, Crete, Greece

    Nikolaos D. Kylafis

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Cernicharo, J. (1991). The Physical Conditions of Low Mass Star Forming Regions. In: Lada, C.J., Kylafis, N.D. (eds) The Physics of Star Formation and Early Stellar Evolution. NATO ASI Series, vol 342. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-3642-6_8

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