Implementation of the Non-equilibrium Ionization Code in ISIS

Details Implementation of the Non-equilibrium Ionization Code in ISIS Implementation of the Non-equilibrium Ionization Code in ISIS

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009cfdd.confe.123j&link_type=abstract

Chandra's First Decade of Discovery, Proceedings of the conference held 22-25 September, 2009 in Boston, MA. Edited by Scott Wo

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The non-equilibrium ionization is present in a wide range of astrophysical phenomena such as colliding winds in X-ray binaries, outflows in AGNs, and shock flows in the IGM. Challenges are significant when applying the non-equilibrium ionization code to the Chandra HETG observations. Parallelism has been used to speed up the calculations. Modular software techniques enable us to compute atomic rates directly in ISIS. We present the implementation of our non-equilibrium ionization code in ISIS based on all the available update atomic data. In addition, we demonstrate several applications to the non-equilibrium ionization plasma for the Chandra HETG observations.

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