Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
University of Maryland
University of Maryland, College Park
Univ. of Maryland
U. Maryland
UMD, USA
University of Maryland at College Park
University of Chicago
Univ. of Chicago
The University of Chicago
University of Maryland, Department of Astronomy, College Park, MD 20742-2421, USA
University of Chicago, Chicago, IL, US
University of Illinois at Urgana-Champaign, Urbana, IL, US
University of Illinois at Urbana-Champaign, Urbana, IL, US
University of Maryland, Department of Astronomy College Park, Maryland 20742-2421, USA
Department of Astronomy and Maryland Astronomy Center for Theory and Computation, University of Maryland, College Park, Maryland 20742-2421, USA
Department of Astronomy, University of Maryland, and the Joint Space Science Institute, College Park, Maryland 20742-2421, USA
Department of Astronomy, University of Maryland, College Park, MD 20742-2421, USA
University of Maryland, Department of Astronomy, College Park, MD 20742, USA
University of Maryland, College Park, USA
Los Alamos National Laboratory, Los Alamos, New Mexico 87544
Univ. Maryland
University of Chicago, Department of Astronomy and Astrophysics, 5640 S. Ellis Ave., Chicago, IL 60637, USA of Chicago, Chicago, IL 60637 USA Alamos National Laboratory, MS-D466, Los, Alamos, USA
Los Alamos National Laboratory, Los Alamos, New Mexico, USA
Illinois Univ., Urbana
UIUC
University of Maryland / College Park, USA
Department of Astronomy, University of Maryland
California Institute of Technology, Pasadena
Illinois Univ., Urbana; NORDITA, Copenhagen, Denmark
Mail Stop D466, Los Alamos National Laboratory, Los Alamos, NM 87545
University of Maryland Department of Astronomy
Illinois, Univer
A Characterization of the Brightness Oscillations During Thermonuclear Bursts From 4U 1636-536
A Comparison of Intermediate Mass Black Hole Candidate ULXs and Stellar-Mass Black Holes
A Computational Study of Core Rotation in Globular Clusters
A Deep Chandra Observation of the X-shaped Radio Galaxy 4C +00.58: A Candidate for Merger-induced Reorientation?
A Determination of the Alignment Angle of Pulsars
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