Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Yale
Yale U
Department of Astronomy, Yale University
Department of Astronomy Yale University New Haven CT
Department of Astronomy, Yale University, P.O. Box 208101, New Haven, CT 06520 University, New Haven, CT
Yale University, Yale, CT, US
Yale University, Department of Astronomy, New Haven 06520-8101, CT, USA
Yale University., New Haven, CT, US
Yale University
Department of Astronomy, Yonsei University, Seoul 120-749, Korea University Observatory, New Haven, CT
Yale University.
Department of Astronomy, Yale University, New Haven, CT 06520-8101
Yale University, New Haven, CT, US
Yale University., New Haven, CT
Astronomy Department, Yale University, P.O. Box 208101, New Haven, CT 06520-8101 of Astronomy, Yale University, P.O. Box 208101, New Haven, CT 06520-8101
Yale University, New Haven, CT 06520-8101, USA
Department of Astronomy, Yale University, New Haven CT, USA
Yale University, New Haven, Connecticut, USA
Department of Astronomy, Yale University, New Haven, CT 06520 University Observatory, New Haven, Connecticut
Department of Astronomy, Yale University, P.O. Box 208101, New Haven, CT 06520-8101, USA
Yonsei Univ. Observatory, Seoul, Korea
Center for Solar and Space Research, Yale University., New Haven, CT, US
the LCID team
Yale Univ.
Yale University Observatory, New Haven, Conn.
Astronomy Department, Yale University, Box 208101, New Haven, CT 06520-8101, USA
Astronomy Department, Yale University
Department of Astronomy, Yale University, P.O. Box 208101, New Haven, CT 06520-8101, USA for Solar and Space
$^7$Li Abundances in Halo Stars: Testing Stellar Evolution Models and the Primordial $^7$Li Abundance
2-D Stellar Evolution Code Including Arbitrary Magnetic Fields. I. Mathematical Techniques and Test Cases
2D solar modeling
3D convection simulations of the outer layers of the Sun using realistic physics
a 2-D Stellar Evolution Code Including Arbitrary Magnetic Fields
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