Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
San Diego State University
Department of Physics, San Diego State University, San Diego, California, USA
Univ. of Munich & LBNL, Berkeley
Lawrence Berkeley National Laboratory, Berkeley, CA, USA
Nuclear Science Division, Institute for Nuclear and Particle Astrophysics, Lawrence Berkeley National Laboratory
University of Munich
Lawrence Berkeley National Laboratory and University of Notre Dame
Department of Physics, University of Notre Dame, IN, USA
California Univ., Berkeley. Lawrence Berkeley Lab, CA.
Institute for Theoretical Physics, Ludwig-Maximilians University, Theresienstr. 37, 80333 Munich, Germany
Nuclear Science Division, Lawrence Berkeley National Laboratory, Berkeley, California 94720
Department of Physics, San Diego State University, 5500 Campanile Drive, San Diego, CA 92182-1233, USA
Department of Physics, San Diego State University, San Diego, CA 92182, USA
Lawrence Berkeley National Laboratory
University of Notre Dame
SDSU
University of Munich, Germany
Department of Physics, San Diego State University, USA
Ludwig-Maximilians Universitaet Muenchen, Germany
Joint Institute for Nuclear Research, 141980 Dubna, Yerevan State University, University of Munich
Technische Univ., Munich, Germany
Department of Physics, University of Notre Dame, IN 46556-5670, USA
Universität München, Am Coulombwall 1, D-85748 Garching bei München, Germany
California Univ., Berkeley. Lawrence Berkeley Lab.
Nuclear Science Division, Lawrence Berkeley Laboratory, University of California
Lawrence Berkeley National Laboratory, University of California, Nuclear Science Division, MS: 70A-3307, Berkeley, CA 94720, USA
California University
Lawrence Berkeley Lab., CA
Nuclear Science Division, Lawrence Berkeley Laboratory, University of California, Berkeley, California 94720
Department of Systems and Computational Neuroscience, Max-Planck-Institute of Neurobiology, Martinsried, Germany
California, University,
Absorption features caused by oscillations of electrons on the surface of a quark star
Analysis of White Dwarfs with Strange-Matter Cores
Application of the improved Hartle method for the construction of general relativistic rotating neutron star models
Are strange stars distinguishable from neutron stars by their cooling behaviour?
Baryon composition and macroscopic properties of neutron stars
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Profile ID: LFWR-SCP-P-7156