The Infrared Emission of Dust in the Born-Again Planetary Nebula Abell 58

Details The Infrared Emission of Dust in the Born-Again Planetary Nebula Abell 58 The Infrared Emission of Dust in the Born-Again Planetary Nebula Abell 58

Mar 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aspc..196...23k&link_type=abstract

Thermal Emission Spectroscopy and Analysis of Dust, Disks, and Regoliths, Proceedings of a meeting held at at The Lunar and Plan

Astronomy and Astrophysics

Astronomy

4

Scientific paper

Single photon heating events of small dust particles result in strong temperature fluctuations and an emission excess in the mid and near infrared with respect to large grains in thermal equilibrium. With an extension of the grain size distribution to smaller grain sizes (between 6 Å and 50 Å) and considering single photon heating events it is possible to describe a number of objects which show this excess. As an example the infrared emission of Abell 58 was successfully modeled.

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