Editing Appendix/References (section)

==21<sup>st</sup> Century==

===CT2000===

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<tr><td align="left">Acknowledgements (p. 1067):<br /><font color="darkgreen">"This work has been supported, in part, by funding from the US National Science Foundation through grant [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=9528424 AST-9528424], and from the NASA Astrophysics Theory Program through grant NAG5-8497.  One of us (J.E.C.) also acknowledges support from the Louisiana Board of Regents' LEQSF under agreement NASA/LSU-(91-96)-01, and through NASA/LaSPACE under grant NGT5-40335.  This work also has been supported in part, by grants of high-performance computing time through the PET program at the NAVOCEANO DoD Major Shared Resource Center in Stennis, Mississippi and through NPACI on machines at the San Diego Supercomputer Center and UT, Austin."
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===CTRS2000===

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<tr><td align="left">Acknowledgements (p. 371):<br /><font color="darkgreen">"HSC would like to thank the LSU (Louisiana State University, U.S.A.) Department of Physics &amp; Astronomy and Prof. J. Frank for providing travel support to attend the 200<sup>th</sup> IAU symposium on Binary Star Formation in Potsdam, Germany, at which the results of this work were first presented.  HSC also thanks Prof. D. A. Browne for his support during the course of this work.  ARPR thanks the Alexander von Humboldt Stiftung and Profs. J. Hinze and F. H. M. Faisal of the University of Bielefeld for their hospitality during the course of this work.  Thanks to E. G. Kalnins for many inspiring communications and for providing the Moon &amp; Spencer (1961b) reference.  Thanks to J. D. Jackson for pointing out the Magnus, Oberhettinger &amp; Soni (1966) reference which gives a further generalization of the Heine identity.  Thanks are also due to J. E. Lambert for several subtle grammatical criticisms and suggestions.  We acknowledge support from NASA through grant NAG5-8497 and from the U.S. National Science Foundation through grant [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=9987344 AST-9987344].  This work also has been supported, in part, by a grant of high-performance computing time on NPACI facilities at the San Diego Supercomputer Center."</font>
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===MTF2002===

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<tr><td align="left">Acknowledgements (p. 148):<br /><font color="darkgreen">"This work has been performed with support from the National Science Foundation through grants [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=9720771 AST-9720771], [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=9528424 AST-9528424], [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=9987344 AST-9987344], and DGE-935507</font> [should be, [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=9355007 DGE-9355007]] <font color="darkgreen">and from the National Aeronautics and Space Administration through the Astrophysics Theory Program grant NAG5-8497.  This research has been supported in part, by grants of high-performance computing time at the National Partnership for Advanced Computing Infrastructure (NPACI) facilities at the San Diego Supercomputer Center and by Louisiana State University's High Performance Computing facilities.  We would also like to acknowledge the many useful comments made by the referee that led to a significant improvement in the contents of this paper."</font>
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===AKM2003===

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<tr><td align="left">Acknowledgements (p. 523):<br /><font color="darkgreen">"The authors would like to thank David Petroff for many valuable discussions.  This work was supported by the Deutsche Forschungsgemeinschaft (DFG-project ME 1820/1)."</font>
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===Hunter2003===

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<tr><td align="left">Acknowledgements (p. 137):<br /><font color="darkgreen">"It is a pleasure to thank George Contoupoulos, and Nikos Voglis and his committee, for organizing a stimulating workshop, and for their hospitality. This work has been supported in part by the National Science Foundation through grant [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=0104751 DMS-0104751]."</font>
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===Hunter2005===

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<tr><td align="left">Acknowledgements (p. 137):<br /><font color="darkgreen">"This work was supported by the National Science Foundation grant [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=0104751 DMS-0104751].  The author declares that he has no competing financial interest."</font>
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===OT2006===

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<tr><td align="left">Acknowledgements (p. 1077):<br /><font color="darkgreen">"We would like to thank Hui Li for insightful and useful discussions at the 47th Meeting of the Division of Plasma Physics of the American Physical Society.  We also thank Juhan Frank, Patrick Motley, Shin Yoshida, and Christian Ott for helpful comments and suggestions.  It is a pleasure to thank Anna Watts for useful conversations at the Eight Division Meeting of High Energy Astrophysics Division of the American Astronomical Society.  We thank an anonymous referee for helpful suggestions.  This work was partially supported by NSF grants [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=0407070 AST 04-07070] and [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=0326311 PHY-0326311].  The computations were performed on the Supermike cluster and the Superhelix cluster at LSU and on the Tungsten cluster at the National Center for Supercomputing Applications (NCSA)."</font>
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===Ou2006===

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<tr><td align="left">Acknowledgements (p. 558):<br /><font color="darkgreen">"I would like to thank Joel Tohline for valuable suggestions, discussions, and for carefully reading through this paper.  I also thank Juhan Frank and Patrick Motl for helpful comments.  It is a pleasure to thank Norman Lebovitz for drawing our attention to the particular analytical expression of the velocity field of Riemann S-type ellipsoids used in this study.  I would also thank Howard Cohl for developing the Poisson solver that was an important ingredient in this work.  I thank the anonymous referee for insightful suggestions on the analysis of our models.  This work was partially supported by National Science foundation grants [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=0407070 AST 04-07070] and [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=0326311 PHY-0326311] and by the [https://cct.lsu.edu Center for Computation and Technology at LSU]."</font>
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===ZEUS-MP2006===

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<tr><td align="left">Acknowledgements (p. 211):<br /><font color="darkgreen">"The release of a vastly redesigned and augmented 'Version 2' of ZEUS-MP was occasioned by ZEUS-MP's adoption by the Terascale Supernova Initiative as a computational platform for simulating core-collapse supernova explosions in multidimensions.  The TSI project, led by Anthony Mezzacappa, provided both the demand and much of the financial support for the effort that created this code.  We are indebted to Tony Mezzacappa for his continued support, enthusiasm, and remarkable patience during the development phase of ZEUS-MP 2.0.  In addition, we gratefully acknowledge the continued support and wise counsel from Frank Graziani at the [https://en.wikipedia.org/wiki/Lawrence_Livermore_National_Laboratory Lawrence Livermore National Laboratory]. This work was supported by SciDAC grants from the DOE Office of Science High-Energy, Nuclear, and Advanced Scientific Computing Research Programs, and by DOE contract W-7405-ENG-48."</font>
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===OTM2007===

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<tr><td align="left">Acknowledgements (p. 1083):<br /><font color="darkgreen">"We would like to thank Lee Lindblom, John Friedman, Nikolaos Stergioulas, Yuk Tung Liu, and Juhan Frank for valuable discussions.  This work was partially supported by NSF grants [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=0407070 AST-0407070] and  [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=0326311 PHY-0326311].  The computations were performed on the Supermike cluster and the Superhelix cluster at LSU, and on the Tungsten cluster at National Center for Supercomputing Applications (NCSA)."</font>
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Click to list chapter(s) on this wiki site that either &hellip; <b>[[Special:WhatLinksHere/Template:OTM2007full|cite]]</b> or <b>[[Special:WhatLinksHere/Template:OTM2007figure|display an image/figure/table from]]</b> this article.
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===PK2007===

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<tr><td align="left">Acknowledgements (p. 710):<br /><font color="darkgreen">"This work was supported in part by the US Department of Energy under contract B523820 to the Center for Astrophysical Thermonuclear Flashes at the University of Chicago.  AYP also expresses gratitude to the Institute for Pure and Applied Mathematics (IPAM), UCLA for support during the semester program 'Grand Challenge Problems in Computational Astrophysics', March-June, 2005.  The authors are grateful to anonymous referees for valuable comments and criticisms."</font>
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===BTZ2012===

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<tr><td align="left">Acknowledgements (p. 2720):<br /><font color="darkgreen">"WHB and AN&#x017B; are grateful to Ramesh Narayan for the discussion that led to the authors pursuing this line of work.  We also thank Peter Eggleton for discussing the formation of giants.  CAT thanks Churchill College for a fellowship."</font>
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===MT2012===

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<tr><td align="left">Acknowledgements (p. 27):<br /><font color="darkgreen">"We acknowledge valuable interactions that we have had with J. Frank, G. Clayton, P. M. Motl, and W. Even over the course of this project.  We also acknowledge the referee for his thorough analysis of our work and his insightful comments.  This work has been supported, in part, by grants [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=0803629 PHY-0803629], [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=0708551 AST-0708551], [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=1006891 EPS-1006891], [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=0963375 OIA-0963375], and [https://www.nsf.gov/awardsearch/simpleSearchResult?queryText=0504507 DGE-0504507] from the U. S. National Science Foundation and, in part, by NASA/ATP grants NNX10AC72G and NNX07AG84G.  This research also has been made possible by grants of high-performance computing time on the TeraGrid (TG-AST090104), at LSU, and across LONI (Louisiana Optical Network Initiative), especially awards loni_astro08 and loni_astro09."</font>
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