Episodic Mass Loss on the Timescale of Thermal Pulses: Radiative Transfer Modeling of the Egg Nebula

Details Episodic Mass Loss on the Timescale of Thermal Pulses: Radiative Transfer Modeling of the Egg Nebula Episodic Mass Loss on the Timescale of Thermal Pulses: Radiative Transfer Modeling of the Egg Nebula

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..313..303s&link_type=abstract

Asymmetrical Planetary Nebulae III: Winds, Structure and the Thunderbird, Proceedings of the conference held 28 July - 1 August

Astronomy and Astrophysics

Astronomy

Scientific paper

We present preliminary results of modeling the parsec-sized dust shell around the Egg Nebula using a version of the 1-d radiative transfer code DUSTY which includes external heating of the dust by the interstellar radiation field. External heating by the interstellar radiation field and increased mass-loss towards the end of the AGB are both necessary for a good fit. Mass-loss episodes can be modeled as enhancements in the density distribution.

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