Radiative transfer modeling of periodic mass-loss enhancement during the AGB phase

Details Radiative transfer modeling of periodic mass-loss enhancement during the AGB phase Radiative transfer modeling of periodic mass-loss enhancement during the AGB phase

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003assl..283..241s&link_type=abstract

In: Mass-losing pulsating stars and their circumstellar matter. Workshop, May 13-16, 2002, Sendai, Japan, edited by Y. Nakada, M

Astronomy and Astrophysics

Astrophysics

Thermal Pulses, Mass Loss, Egg Nebula, Dust

Scientific paper

We present radiative transfer (RT) models of the dust shell around the
Egg nebula using the 1-d RT code DUSTY which has been modified to
include heating by ISRF.

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