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The Iron Project: Atomic Data for Fe I-Fe VI

Published online by Cambridge University Press:  12 April 2016

Manuel A. Bautista ,
Sultana N. Nahar ,
Jianfang Peng ,
Anil K. Pradhan  and
Hong Lin Zhang
Manuel A. Bautista
Affiliation:
Department of Astronomy, Ohio State University, 174 West 18th Avenue, Columbus, OH 43210, USA
Sultana N. Nahar
Affiliation:
Department of Astronomy, Ohio State University, 174 West 18th Avenue, Columbus, OH 43210, USA
Jianfang Peng
Affiliation:
Department of Astronomy, Ohio State University, 174 West 18th Avenue, Columbus, OH 43210, USA
Anil K. Pradhan
Affiliation:
Department of Astronomy, Ohio State University, 174 West 18th Avenue, Columbus, OH 43210, USA
Hong Lin Zhang
Affiliation:
Department of Astronomy, Ohio State University, 174 West 18th Avenue, Columbus, OH 43210, USA

Abstract

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Recent progress in large scale computations of photoionization cross sections, radiative transitions probabilities, and collision strengths for the lowest ionization stages of Iron, i.e., Fe I-VI, are reported. These results are part of an international collaboration called the IRON Project. The present results exhibit large differences with respect to data currently in use and is expected to be of importance in the study of astrophysical objects in the UV and the EUV.

Type
XIII. Plasma Diagnostics
Information
International Astronomical Union Colloquium , Volume 152: Astrophysics in the Extreme Ultraviolet , 1996 , pp. 577 - 581
Copyright
Copyright © Kluwer 1996

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