Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002a%26a...390..779b&link_type=abstract
Astronomy and Astrophysics, v.390, p.779-782 (2002)
Astronomy and Astrophysics
Astrophysics
45
Molecular Data, Astronomical Data Basess, Stars: Atmospheres, Stars: Low-Mass, Brown Dwarfs, Infrared: Stars
Scientific paper
New collision-induced absorption data of H2 pairs at temperatures between 400 K and 1000 K are presented here for the first time. They are based on a careful interpolation and extension of the existing `low' temperature data, which were suited for use in planetary atmospheric modelling. The new data are aimed to help in modelling the coolest halo white dwarfs, the coolest M dwarfs, the L- and T- type dwarf stars, as well as brown dwarfs and ``hot jupiters''. In addition, for the convenience of the future users, the already existing low temperature (60 K to 400 K) data are provided, in a consistent and user friendly tabular form. The data above 1000 K, which already existed, form a continuous sequence with the new data presented here. The total data set from 60 K to 7000 K and frequencies from 0 cm-1 to <=17 000 cm-1 (computed for every 10 cm-1) is now located at www.astro.ku.dk/ ~ aborysow/programs.
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