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Atomic Data for Stellar Nucleosynthesis

Published online by Cambridge University Press:  27 October 2016

Christopher Sneden ,
James E. Lawler ,
Elizabeth A. Den Hartog  and
Michael E. Wood
Christopher Sneden
Affiliation:
Department of Astronomy and McDonald Observatory, The University of Texas, Austin, TX 78712 email: [email protected]
James E. Lawler
Affiliation:
Department of Physics, University of Wisconsin-Madison, 1150 University Ave., Madison, WI 53706 email: [email protected], [email protected], [email protected]
Elizabeth A. Den Hartog
Affiliation:
Department of Physics, University of Wisconsin-Madison, 1150 University Ave., Madison, WI 53706 email: [email protected], [email protected], [email protected]
Michael E. Wood
Affiliation:
Department of Physics, University of Wisconsin-Madison, 1150 University Ave., Madison, WI 53706 email: [email protected], [email protected], [email protected]
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Abstract

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Stellar chemical composition analyses can only yield reliable abundances if the atomic transition parameters are accurately determined. During the last couple of decades a renewed emphasis on laboratory spectroscopy has produced large sets of useful atomic transition probabilities for species of interest to stellar spectroscopists. In many cases the transition data are of such high quality that they play little part in the abundance uncertainties. We summarize the current state of atomic parameters, highlighting the areas of satisfactory progress and noting places, where further laboratory progress will be welcome.

Keywords

atomic datastars: abundancesstars: Population II
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29A: Astronomy in Focus , August 2015 , pp. 287 - 290
Copyright
Copyright © International Astronomical Union 2016 

References

Biémont, É., Blagoev, K., Engström, L., et al. 2011, MNRAS, 414, 3350 Google Scholar
Boyd, R. N., Famiano, M. A., Meyer, B. S., et al. 2012, ApJL, 744, L14 Google Scholar
Den Hartog, E. A., Ruffoni, M. P., Lawler, J. E., et al. 2014, ApJS, 215, 23 CrossRefGoogle Scholar
Den Hartog, E. A., Lawler, J. E., Sobeck, J. S., Sneden, C., & Cowan, J. J. 2011, ApJS, 194, 35 Google Scholar
Engström, L., Lundberg, H., Nilsson, H., Hartman, H., & Bäckström, E. 2014, A&A, 570, A34 Google Scholar
Fedchak, J. A. & Lawler, J. E. 1999, ApJ, 523, 734 Google Scholar
Griffin, R., Gustafsson, B., Vieira, T., & Griffin, R. 1982, MNRAS, 198, 637 CrossRefGoogle Scholar
Gurell, J., Nilsson, H., Engström, L., et al. 2010, A&A, 511, A68 Google Scholar
Ivans, I. I., Simmerer, J., Sneden, C., et al. 2006, ApJ, 645, 613 Google Scholar
Johansson, S., Derkatch, A., Donnelly, M. P., et al. 2002, Phys. Scr. T, 100, 71 Google Scholar
Kobayashi, C., Karakas, A. I., & Umeda, H. 2011, MNRAS, 414, 3231 Google Scholar
Lawler, J. E., Guzman, A., Wood, M. P., Sneden, C., & Cowan, J. J. 2013, ApJS, 205, 11 CrossRefGoogle Scholar
Lawler, J. E., Sneden, C., & Cowan, J. J. 2015, ApJS, 220, 13 CrossRefGoogle Scholar
Lawler, J. E., Wood, M. P., Den Hartog, E. A., et al. 2014, ApJS, 215, 20 Google Scholar
Malcheva, G., Blagoev, K., Mayo, R., et al. 2006, MNRAS, 367, 754 Google Scholar
Meléndez, J. & Barbuy, B. 2009, A&A, 497, 611 Google Scholar
Mullman, K. L., Cooper, J. C., & Lawler, J. E. 1998, ApJ, 495, 503 CrossRefGoogle Scholar
Nilsson, H., Ljung, G., Lundberg, H., & Nielsen, K. E. 2006, A&A, 445, 1165 Google Scholar
O'Brian, T. R., Wickliffe, M. E., Lawler, J. E., Whaling, W., & Brault, J. W. 1991, Journal of the Optical Society of America B Optical Physics, 8, 1185 Google Scholar
Pickering, J. C., Johansson, S., & Smith, P. L. 2001, A&A, 377, 361 Google Scholar
Pickering, J. C., Donnelly, M. P., Nilsson, H., Hibbert, A., & Johansson, S. 2002, A&A, 396, 715 Google Scholar
Placco, V. M., Beers, T. C., Ivans, I. I., et al. 2015, ApJ, 812, 109 CrossRefGoogle Scholar
Ruffoni, M. P., Den Hartog, E. A., Lawler, J. E., et al. 2014, MNRAS, 441, 3127 Google Scholar
Siqueir AMello, C., Spite, M., Barbuy, B., et al. 2013, A&A, 550, A122 Google Scholar
Sneden, C., Cowan, J. J., & Gallino, R. 2008, ARA&A, 46, 241 Google Scholar
Sneden, C., Cowan, J. J., Pignatari, M., Kobayashi, C., Lawler, J. E., Den Hartog, E. A., & Wood, M. P. 2015, ApJS, submittedGoogle Scholar
Sneden, C., Lawler, J. E., Cowan, J. J., Ivans, I. I., & Den Hartog, E. A. 2009, ApJS, 182, 80 Google Scholar
Sobeck, J. S., Lawler, J. E., & Sneden, C. 2007, ApJ, 667, 1267 Google Scholar
Wood, M. P., Lawler, J. E., Den Hartog, E. A., Sneden, C., & Cowan, J. J. 2014a, ApJS, 214, 18 Google Scholar
Wood, M. P., Lawler, J. E., Sneden, C., & Cowan, J. J. 2013, ApJS, 208, 27 CrossRefGoogle Scholar
Wood, M. P., Lawler, J. E., Sneden, C., & Cowan, J. J. 2014b, ApJS, 211, 20 Google Scholar