Probing the formation mechanism of prestellar cores and the origin of the imf: first results from the herschel gould belt survey

Publisher: Edp Sciences

E-ISSN: 1638-1963|52|issue|167-172

ISSN: 1633-4760

Source: EAS Publications Series, Vol.52, Iss.issue, 2011-11, pp. : 167-172

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Abstract

We summarize the first results from the Herschel Gould Belt survey, one of the largest key projects with the Herschel Space Observatory. Our early findings confirm the existence of a close relationship between the prestellar core mass function (CMF) the stellar initial mass function (IMF). Furthermore, they suggest a scenario according to which the formation of prestellar cores occurs in two main steps: 1) complex networks of long, thin filaments form first, probably as a result of interstellar MHD turbulence; 2) the densest filaments then fragment and develop prestellar cores via gravitational instability.

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