Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Harvard-Smithsonian Center for Astrophysics
U. of Arizona
University of Arizona
Univ. of Illinois at Urbana-Champaign
U. Arizona
U.Arizona
MIT
IAS / Arizona
Harvard-Smithsonian CfA
University of Illinois
Physics Dept., University of Arizona, Tucson
Physics Department, University of Arizona
Harvard-Smithsonian CFA
University of Arizona, Tucson, AZ
Department of Physics, University of Arizona, Tucson, Arizona 85721, USA; Department of Astronomy, University of Arizona, Tucson, Arizona 85721, USA
University of Illinois at Urbana-Champaign, Urbana, IL, US
Physics and Astronomy Departments, University of Arizona, 1118 East Fourth Street, Tucson, AZ 85721
Harvard, Astrophysics
University of Illinois at Urbana-Champaign
Department of Astronomy, University of Arizona, 933 N. Cherry Ave., Tucson, AZ 85721, USA
MIT / IAS
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, Massachusetts 02138
Princeton
Harvard / CfA
Dept. of Physics, Univ. of Arizona
IAS Princeton
CfA,MIT
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, USA of Engineering and Natural Sciences, Sabancı University, Orhanlı, Tuzla, Istanbul 34956, Turkey; Physics and Astronomy Departments, 1118 E. 4th Street, Tucson, AZ, 85721, USA
IAS and University of Arizona
Institute for Advanced Study, School of Natural Sciences
University of Arizona, 1118 E. 4th st., Tucson, AZ 85721
University of Arizona, Tuscon
University of Arizona -Department of Physics
Physics and Astronomy Departments, University of Arizona
University of Arizona, Physics Department, 1118 E. 4th str., Tucson, AZ 85721, USA
A Local Model for Angular Momentum Transport in Accretion Disks Driven by the Magnetorotational Instability
A Metric for Rapidly Spinning Black Holes Suitable for Strong-Field Tests of the No-Hair Theorem
A multi-Lorentzian timing study of the atoll sources 4U 0614+09 and 4U 1728-34
A Ray-Tracing Algorithm for Spinning Compact Object Spacetimes with Arbitrary Quadrupole Moments. I. Quasi-Kerr Black Holes
A Ray-Tracing Algorithm for Spinning Compact Object Spacetimes with Arbitrary Quadrupole Moments. II. Neutron Stars
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