Model Atmospheres and Spectra for Extrasolar Giant Planets

Details Model Atmospheres and Spectra for Extrasolar Giant Planets Model Atmospheres and Spectra for Extrasolar Giant Planets

Jan 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000stin...0186235f&link_type=abstract

Technical Report, Space Physics Research Inst. Sunnyvale, CA United States

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Applications

Brown Dwarf Stars, Extrasolar Planets, Opacity, Spectrum Analysis, Astronomical Models, Applications Programs (Computers), Data Correlation, Space Observations (From Earth), Planetary Atmospheres

Scientific paper

In the past few years much new observational data has become available for brown dwarfs and extra solar planets. Not only are new objects being discovered but the availability of higher resolution spectra is improving. This allows a better comparison between the models and the available data, and places new constraints on the models which now have to be made more physically realistic in order to better interpret the observations. Under this grant, an array of new opacities were calculated and successfully applied to a variety of physical situations that were used as input to model available observations of brown dwarfs and extra solar giant planets.

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