The evolution of young stellar object disks and their environment

Details The evolution of young stellar object disks and their environment The evolution of young stellar object disks and their environment

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991plas.rept..117s&link_type=abstract

In NASA, Washington, Reports of Planetary Astronomy, 1991 p 117-120 (SEE N92-12792 03-89)

Astronomy and Astrophysics

Astronomy

Accretion Disks, G Stars, Main Sequence Stars, Occurrences, Stellar Mass, Stellar Mass Accretion

Scientific paper

The main efforts were directed towards determining the frequency of disk
occurrence and the timescales for disk evolution for solar-type and
intermediate mass stars. The results of the investigation showed that
optically thick disks are accretion disks. The projected accomplishments
are also discussed.

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