High-Temperature Optical Constants of Dust Analogues for the Solar Nebula

Details High-Temperature Optical Constants of Dust Analogues for the Solar Nebula High-Temperature Optical Constants of Dust Analogues for the Solar Nebula

2012-01-09

arxiv.org/abs/1201.1801v1

Astronomy and Astrophysics

Astrophysics

Earth and Planetary Astrophysics

4 pages, 3 figures, Contribution for the ECLA proceedings (European Conference on Laboratory Astrophysics)

Scientific paper

The dust in protoplanetary disks is influenced by a lot of different processes. Besides others, heating processes are the most important ones: they change not only the physical and chemical properties of dust particles, but also their emission spectra. In order to compare observed infrared spectra of young stellar systems with laboratory data of hot (up to 700{\deg}C) circumstellar dust analogues, we investigate materials, which are important constituents of dust in protoplanetary disks. We calculated the optical constants by means of a simple Lorentzian oscillator fit and apply them to simulations of small-particle emission spectra in order to compare our results with real astronomical spectra of AGB-stars and protoplanetary disks.

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