Small-scale properties of low-mass Class 0 protostars: digging into the memory of accretion processes

Details Small-scale properties of low-mass Class 0 protostars: digging into the memory of accretion processes Small-scale properties of low-mass Class 0 protostars: digging into the memory of accretion processes

Nov 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011eas....51..191m&link_type=abstract

EAS Publications Series, Volume 51, 2011, pp.191-209

Physics

Scientific paper

In this lecture, we briefly present the main models currently proposed to describe the collapse of prestellar dense cores and the formation of young Class 0 protostars. An empirical evolutionary sequence for the formation of low-mass stars is described. Then, the typical properties of Class 0 protostars are reviewed and the question of their structure at small scales is adressed through the question of circumstellar disks.

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