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Atomic Physics Data for Stellar Atmospheres Research

Published online by Cambridge University Press:  26 May 2016

Charles R. Cowley ,
Saul J. Adelman  and
Donald J. Bord
Charles R. Cowley
Affiliation:
University of Michigan, Ann Arbor, MI 48109-1090, USA
Saul J. Adelman
Affiliation:
The Citadel, Charleston, SC 29409-0270, USA
Donald J. Bord
Affiliation:
University of Michigan, Dearborn, MI 48128-1491, USA

Abstract

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The review will cover the following topics: (1) Ionization energies; (2) Partition functions; (3) Sources of data for atomic and ionic wavelengths, transition probabilities, and broadening parameters, including nuclear effects (hfs and isotope shifts); (4) Opacities from photoionization of abundant elements (atoms and atomic ions) with emphasis on integration of TOPBASE material; and (5) Data bases for diatomic molecules. We emphasize topics of direct relevance to the synthesis of stellar spectra, primarily within the domain where LTE is useful. Additional parameters, such as line-broadening parameters, or excitation cross sections are not reviewed.

Information

Type
Session E. Comparison with Observations
Information
Symposium - International Astronomical Union , Volume 210: Modelling of Stellar Atmospheres , 2003 , pp. 261 - 272
Copyright
Copyright © Astronomical Society of the Pacific 2003 

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