Infall in Young Stars

Details Infall in Young Stars Infall in Young Stars

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997cokon.100..333n&link_type=abstract

Communications of the Konkoly Observatory, No. 100 (Vol. XII, 2), p. 333-340 (1997)

Computer Science

Scientific paper

I discuss in this paper three examples of gas infall in pre-main sequence stars and in very young main-sequence stars. Although the fraction of mass accreted by the star in these later phases is small in comparison to earlier phases of star formation, by investigating the origin and properties of the infalling matter we can address a number of problems, from the properties of accretion disks to the early phases of the formation of solar systems.

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