Gas - surface interactions in star-forming
regions
David Williams
University College London
Friday, 15 October 2004
10:00 am, Pratt Conference Room
Harvard-Smithsonian Center for Astrophysics
Abstract:
In denser regions of interstellar space, such as those in
star-forming regions, the interactions between gas atoms and
molecules with dust grain surfaces become more significant. An
example of this is the growth of ice coatings on dust grains
by the hydrogenation of oxygen atoms on surfaces in regions above
a certain critical visual extinction. Surface processes may in
some circumstances dominate gas-phase processes. There is a need
for reliable information on adsorption, desorption, reaction,
and also on the solid-state processing of amorphous ices. In
my talk I shall describe recent studies of situations in which
the gas-surface interactions are likely to be important. These
may include hot cores in regions of massive star formation, clumpy
models of molecular clouds in regions of low mass star formation,
and the interaction of stellar jets with dense cores within clumpy
clouds.
|