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Protoplanetary disk dispersal
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2026-10-20
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Removal of disk
gas
by
accretion
onto the host
star
,
winds
and
photoevaporation
. The finite availability of
gas
limits which
solid
cores can acquire massive envelopes. The disk'
s
evolutionary state
matters
more than
a
single universal
dispersal
time
.
Incoming links
(5)
Past exam of the exoplanets and Planetary Systems course of the University of Cambridge
/
2015
/
Paper 1
/
2
/
Solution
Past exam of the exoplanets and Planetary Systems course of the University of Cambridge
/
2016
/
Paper 1
/
2
/
Solution
Past exam of the exoplanets and Planetary Systems course of the University of Cambridge
/
2016
/
Paper 1
/
3
/
a
/
Solution
Past exam of the exoplanets and Planetary Systems course of the University of Cambridge
/
2016
/
Paper 1
/
3
/
c
/
Solution
Runaway gas accretion
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