Modeling dust emission in PN IC 418
We investigated the infrared (IR) dust emission from PN IC 418, using a detailed model controlled by a previous determination of the stellar properties and the characteristics of the photoionized nebula, keeping as free parameters the dust types, amounts, and distributions relative to the distance of the central star. The model includes the ionized
Gómez-Llanos, V. et al.
Fecha de publicación:
9
2018