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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 

References

Bolton, C. T. 1970, Ap. J., 161, 1187.Google Scholar
Bord, D. J., and Cowley, C. R. 2002, Solar Phys., in press. (astro-ph/0207585) Google Scholar
Campbell-Miller, M. D., and Simard, B. 1996, J. Opt. Soc. Am., B, 13, 2115.Google Scholar
Corliss, C. H. 1969, J. Res. NBS, 73A, 277.Google Scholar
Cowan, J. J., Sneden, C., Burles, S., Ivans, I. I., Beers, T. C., Truran, J. W., Lawler, J. E., Primas, F., Fuller, G. M., Pfeiffer, B., and Kratz, K.-L. 2002, Ap. J., in press. (astro-ph/0202429) Google Scholar
Cowan, R. D. 1981, The Theory of Atomic Structure and Spectra, (Berkeley: Univ. California Press).Google Scholar
Cowley, C. R., and Barisciano, L. P. Jr. 1994, The Observatory, 114, 308.Google Scholar
Daems, R., Biémont, E., and Grevesse, N. 1984, unpublished results. Google Scholar
Dappen, W. 2000, in Allen's Astrophysical Quantities, 4th ed., ed. Cox, A. N., Chapter 3, pp. 36–38.Google Scholar
Ekberg, J. O., Kling, R., and Mende, W. 2000, Physica Scripta, 61, 146. (EKM) CrossRefGoogle Scholar
Fuhr, G. A., Martin, G. A., and Wiese, W. L. 1988, J. Phys. Chem. Ref. Data., Vol. 17, Suppl. 4.Google Scholar
Gluck, G. G., Bordarier, V., Bauche, J., and van Kleef, T. A. M. 1964, Physica, 30, 2068.Google Scholar
Griem, H. R. 1997, Principles of Plasma Spectroscopy, (Cambridge: University Press).CrossRefGoogle Scholar
Halenka, J., and Madej, J. 2002, Acta Astron., 52, 199.Google Scholar
Henderson, M., Irving, R. E., Matulioniene, R., Curtis, L. J., Ellis, D. G., Wahlgren, G. M., and Brage, T. 1999, Ap. J., 520, 805.CrossRefGoogle Scholar
Irwin, A. W. 1981, Ap. J. Suppl., 45, 621.CrossRefGoogle Scholar
Kupka, F., Piskunov, N. E., Ryabchikova, T. A., Stempels, H. C., and Weiss, W. W. 1999, A&AS, 138, 119.Google Scholar
Kurucz, R. L. 1994, CDRom No. 22, (Cambridge MA: Smith. Ap. Obs.) See also his web site, url above.Google Scholar
Laun, D. D., and Corliss, C. H. 1968, J. Res. NBS, 72A, 609.Google Scholar
Leckrone, D. S., Proffitt, C. R., Wahlgren, G. M., Johansson, S. G., and Brage, T. 1999, Astron. J., 117, 1454.Google Scholar
Martin, W. C., Zalubas, R., and Hagan, L. 1978, Atomic Energy Levels–The Rare Earth Elements, NSRDS-NBS 60 (Washington: U. S. Gov. Print. Off.).CrossRefGoogle Scholar
Moore, C. E. 1958, Atomic Energy Levels, Vol. III, NBS Circ. 467 (Washington: U. S. Gov. Print. Off.). (AEL) Google Scholar
Moore, C. E. 1970, Ionization Potentials and Ionization Limits Derived from the Analysis of Optical Spectra, NSRDS-NBS 34, (Washington: U. S. Gov. Print. Off.).Google Scholar
Peach, G. 1970, Mem. R.A.S., 73, 1.Google Scholar
Prieto, C. A. 2000, http://hebe.as.utexas.edu/at/at.cgi Google Scholar
Sansonetti, J., and Martin, W. C. 2000, http://physics.nist.gov/PhysRefData/Handbook/index.html Google Scholar
Seaton, M. J., 1987, J. Phys. B., 20, 6363.Google Scholar
Shadmi, Y., and Caspi, E. 1968, J. Res. NBS, 72A, 757.CrossRefGoogle Scholar
Traving, G., Baschek, B., and Holweger, H. 1966, Abh. Hamburger Sternw., 8, 3.Google Scholar
Trees, R. E. 1958, Phys. Rev., 112, 165.Google Scholar
van Kleef, T. A. M. and Klinkenberg, P. F. A. 1961, Physica, 27, 83.Google Scholar
Van't Veer-Menneret, C. 1961, CR, 253, 380.Google Scholar
Wahlgren, G. M., Johansson, S. G., Litzén, U., Gibson, N. D., Cooper, J. C., Lawler, J. E., Leckrone, D. S., and Engleman, P. 1997, Ap. J., 475, 380.Google Scholar
Wahlgren, G. M., Leckrone, D. S., Brage, T., Proffitt, C. R., and Johansson, S. G. 1998, in The Scientific Impact of the Goddard High Resolution Spectrograph, eds. Brandt, J. C., Ake, T. B. III, and Petersen, C. C., ASP Conf. Ser. 143 (San Francisco: ASP), p. 330.Google Scholar
Wyart, J.-F. 1978, Physica Scripta, 18, 87.Google Scholar