Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S283(7), p. 452-453, 2011
DOI: 10.1017/s174392131201188x
Full text: Unavailable
AbstractWe construct a detailed model for the IR dust emission from the PN IC 418. We succeed to reproduce the emission from 2 to 200 μm. We can determine the amount of emitting dust as well as its composition, and compare to the depletion of elements determined for the photoionized region.