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Keywords

INFRARED: ISM: LINES
ISM:DUST
ISM: PLANETARY NEBULAE: NGC 6302

How to Cite

Photoionization dusty models of the planetary nebula NGC 6302. (2001). Revista Mexicana De Astrofísica Y Astronomía Serie De Conferencias, 10(1), 30-33. https://astronomia.unam.mx/journals/rmxac/article/view/2001rmxac..10...30b
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Abstract

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.