Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976ap%26ss..43..239s&link_type=abstract
Astrophysics and Space Science, vol. 43, Aug. 1976, p. 239-248.
Astronomy and Astrophysics
Astrophysics
5
Galactic Radiation, Granular Materials, Interstellar Matter, Particle Size Distribution, Pressure Effects, Radiation Pressure, Astronomical Models, Distribution Functions, Gravitational Effects, Particle Motion
Scientific paper
It is proposed that radiation pressure generated by sources within the Galaxy is capable of driving grains out of interstellar clouds. The force due to the radiation is analyzed along with the 'viscous' resistance of a spherical grain to the motion, the gravitational force of an interstellar cloud, and the motion of a grain relative to the cloud. Calculations are carried out for the mean sizes to which grains will grow before being expelled and for the corresponding grain-size distribution function. It is concluded that the growth of grains in the presence of the investigated expulsion mechanism is limited to sizes consistent with those deduced from observations.
Simons Stephen
Williams Iwan P.
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