Issue |
A&A
Volume 400, Number 3, March IV 2003
|
|
---|---|---|
Page(s) | 1161 - 1162 | |
Section | Atomic, molecular, and nuclear data | |
DOI | https://doi.org/10.1051/0004-6361:20030100 | |
Published online | 07 March 2003 |
The H2–H infrared absorption bands at temperatures from 1000 K to 2500 K
The University of Texas at Austin, Physics Department, 1 University Station C1600, Austin, TX 78712-0264, USA e-mail: frommhold@physics.utexas.edu
Corresponding author: M. Gustafsson, magnus@physics.utexas.edu
Received:
31
October
2002
Accepted:
14
January
2003
H2–H collision-induced absorption spectra are computed for temperatures from 1000 K to 2500 K and frequencies from 100 cm-1 to 10 000 cm-1. The calculations are quantum mechanical and the isotropic potential approximation has been applied. The computed absorption in the fundamental band agrees roughly with the one determined by Patch (1974). However, the absorption in the translational band, which has not been obtained before, is significantly stronger than in the fundamental band.
Key words: molecular processes / infrared: stars / line: profiles / radiation mechanisms: thermal / scattering / stars: atmospheres
© ESO, 2003
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.