Photoionization dusty models of the planetary nebula NGC 6302

Details Photoionization dusty models of the planetary nebula NGC 6302 Photoionization dusty models of the planetary nebula NGC 6302

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001rmxac..10...30b&link_type=abstract

The Seventh Texas-Mexico Conference on Astrophysics: Flows, Blows and Glows (Eds. William H. Lee and Silvia Torres-Peimbert) Rev

Astronomy and Astrophysics

Astrophysics

Infrared: Ism: Lines, Ism:Dust, Ism: Planetary Nebulae: Ngc 6302

Scientific paper

Using photoionization calculations with dust, we model the high
excitation infrared lines of NGC 6302. This object is a high excitation
bipolar planetary nebula of Peimbert type I. We find that including the
dust results in a significantly hotter nebula.

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