Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientist
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
Scientist
Univ. of California, Berkeley
University of California, Berkeley
UC Berkeley
Berkeley
California, University, Berkeley and Livermore
Department of Astronomy, UCB
California, University, Berkeley; Lawrence Livermore National Laboratory, Livermore, CA
University of California, Berkely, CA, US
University of Calilfornia, Berkeley, CA, US
UC, Berkeley
Astronomy Department, University of California at Berkeley
California Univ., Berkeley; Lawrence Livermore National Lab., Livermore
Department of Astronomy and Department of Physics, University of California, Berkeley, CA 94720, USA
Institute for Theoretical Physics, University of California, Santa Barbara, California 93106
University of CaliforniaSusan M.LeaPhysics and Astronomy Department, San Francisco State University San Francisco, CA 94132
Department Astronomy, 601 Campbell Hall, Un California, Berkeley, California 94720; Department Physics, Un California, Berkeley, California 94720; Theoretical Astrophysics Center, Un California, Berkeley, California 94720
Department of Astronomy, 601 Campbell Hall, Univeresiy of California, Berkeley, CA. 9472; Theoretical Astrophysics Center, University of California, Berkeley, CA 94720; Department of Physics, University of California, Berkeley, CA 94720 Livermore National Laboratory, Livermore; California, University, Berkeley
Commissariat a l'Energie Atomique, Saclay, France
California, University, Berkeley; Lawrence Livermore National Laboratory, Livermore
Princeton University, Princeton, NJ, US
Astronomy Dep. U.C. Berkeley
Astronomy Department, UC Berkeley
UCB
California Univ., Berkeley.
California Univ., Berkeley
California, University, Berkeley, Calif.
California, University, Berkeley, Calif; Cambridge University, Cambridge, England
University of California
University of
A Multiple Pulsar Model for QSOs and Seyfert Nuclei.
A multiple pulsar model for quasi-stellar objects and active galactic nuclei
A reprocessing model for the ultraviolet and optical light from 4U 1820-30
A Reprocessing Model for the UV and Optical Light from 4U1820--30
A Shocked Pulsar Wind Model of the Crab Nebula's Wisps
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Profile ID: LFWR-SCP-P-51513