Data Sources
Opacities
- Mean Opacities can be provided for hydrogen-rich, molecule dominated gases.
- Rosseland and Planck mean gas-phase opacity tables from Helling & Lucas (2009)
- ReadMe for content and structure of data files
- Mean Opacity Tables for [M/H]'=-2.0 (tar-file, unzip with -xvzf)
- Mean Opacity Tables for [M/H]'=-3.0 (tar-file)
- Mean Opacity Tables for [M/H]'=-4.0 (tar-file)
- Mean Opacity Tables for [M/H]'=-5.0 (tar-file)
- The means are based on a data collection from the Copenhagen SCAN data base and the HITRAN data base.
- Mean opacities have been calcualed for
AGB stars (Helling et al. 2000),
planetary atmospheres (Frakis 2001),
protoplanetary disks (Semenov et al. 2003),
planetary and stellar evolution (Helling & Lucas 2009)
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Literature:
Helling & Lucas 2008 (MNRAS, accepted, on astroph)
Semenov, Henning, Helling, Ilgner, Sedlmayr 2003, A&A 410, 611
Helling, Winters, Sedlmay 2000, A&A 358, 651-664
Schnabel (2001) - Master Thesis, TU Berlin, Germany
Helling (1999) - PhD Theses, TU Berlin, Germany
- Observed molecules in the ISM, comets, planetary
atmospheres (except the Earth), as well as several other molecules,
not yet detected, but which are believed to be of astrophysical
importance:
CONSTANTS FOR MOLECULES OF ASTROPHYSICAL INTEREST IN THE GAS PHASE: PHOTODISSOCIATION, MICROWAVE AND INFRARED SPECTRA.
by Jacques Crovisier (Observatoire de Paris-Meudon)
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Tables of Optical Constants
(Astrophysical Institute, University Jena)
10.06.2009
Christiane Helling