Implications of Dust for the Radiation Spectrum of Shell-Type PN Models

Details Implications of Dust for the Radiation Spectrum of Shell-Type PN Models Implications of Dust for the Radiation Spectrum of Shell-Type PN Models

Feb 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002rmxac..12..164k&link_type=abstract

Ionized Gaseous Nebulae, a Conference to Celebrate the 60th Birthdays of Silvia Torres-Peimbert and Manuel Peimbert, Mexico City

Astronomy and Astrophysics

Astronomy

Circumstellar Matter, Line: Profiles, Binaries: Symbiotic, Planetary Nebulae: General, Stars: Agb And Post-Agb

Scientific paper

We have modeled the dust in extended PNe and found that the traditional
methods used to derive dust temperature and dust-to-gas ratio from IRAS
25 and 60 mu m fluxes can be subject to large errors.

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