The cause of intermittent outbursts in radiative hydrodynamic stellar models

Details The cause of intermittent outbursts in radiative hydrodynamic stellar models The cause of intermittent outbursts in radiative hydrodynamic stellar models

Jan 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.140..431t&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 140, no. 2, Jan. 1988, p. 431-434.

Astronomy and Astrophysics

Astrophysics

5

Hydrodynamic Equations, Stellar Models, Supergiant Stars, Luminous Intensity, Radiation Pressure

Scientific paper

The cause of intermittent outbursts found in the pulsations of radiative
hydrodynamic stellar models is discussed. The effect of radiation
pressure, which will not yield the outbursts in convective models, can
be a candidate process for the phenomena.

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