Formation and evolution of dust clumps around cool stars

Details Formation and evolution of dust clumps around cool stars Formation and evolution of dust clumps around cool stars

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003assl..283..245n&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

Circumstellar Matter, Cool Stars, Dust

Scientific paper

In order to model the possibly cloudy circumstellar envelopes of AGN and
post-AGB stars we developed a code describing the coupling between
radiative transfer and time-dependent heterogeneous growth and
evaporation of carbon grains.

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