Are collisions with neutral hydrogen important for modeling the second solar spectrum of Ti I and Ca II?
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20077424/pdf
Reference29 articles.
1. Cox, A. N. 2000, Allen's Astrophysical Quantities, 4th Ed. (New York: Springer Verlag and AIP Press)
2. Collisional depolarization of molecular lines. Application to the SiO+H isotropic collisions
3. Semi-classical theory of collisional depolarization of spectral lines by atomic hydrogen I. Application to p states of neutral atoms
4. Collisional depolarization and transfer rates of spectral lines by atomic hydrogen
5. Collisional depolarization of the lines of complex atoms/ions by neutral hydrogen
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