Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...232..636l&link_type=abstract
Astrophysical Journal, Part 1, vol. 232, Sept. 1, 1979, p. 636-648.
Astronomy and Astrophysics
Astrophysics
10
Atomic Excitations, Ionic Collisions, Isoelectronic Sequence, Proton Impact, Alpha Particles, Beryllium, Magnesium, Scattering Cross Sections, Transition Probabilities
Scientific paper
Proton collisional excitation cross sections and rate constants are presented for transitions between the 3P(J) fine-structure levels of the lowest-lying sp configurations in a number of astrophysically important ions belonging to the Be and Mg isoelectronic sequences. The calculations were made by direct integration of the Schroedinger equation resulting from semiclassical Coulomb excitation theory. The cross sections and rate constants for the 3P(J) transitions in the lowest-lying P(2) configurations are expected to be similar to those for the corresponding sp configuration transitions, and this is illustrated for C III. For the high-temperature ion Ca XVII alpha particle excitation is shown to be unimportant for situations involving ordinary values of the He/H abundance ratio. A simple, but apparently accurate method for determining certain radial integrals for low-lying excited configurations is proposed.
Brown Tim
Landman Donald A.
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