Atomic physics for modeling of astrophysical plasmas

Details Atomic physics for modeling of astrophysical plasmas Atomic physics for modeling of astrophysical plasmas

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..381...47s&link_type=abstract

The tenth American Physical Society topical conference on atomic processes in plasmas. AIP Conference Proceedings, Volume 381,

Astronomy and Astrophysics

Astrophysics

2

Fundamental Aspects Of Astrophysics

Scientific paper

This paper describes the various types of ionization equilibrium applicable to the modeling of astrophysical plasmas, particularly collisional ionization and photoionization equilibrium. Modern astrophysical studies rely heavily on atomic data for derivation of physical parameters from observations, as well as for theoretical modeling. I will describe the current state of atomic data for two areas: (1) Abundances and absorption-line oscillator strengths; (2) Hot plasma ionization and emission.

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