Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientist
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
Scientist
P.N.Lebedev Physical Institute, Moscow, Russia
Department of Physics, University of Hong Kong, Hong Kong, China
P. N. Lebedev Physical Institute, Leninskii pr. 53, 117924 Moscow, Russia
Akademiia Nauk SSSR, Fizicheskii Institut, Moscow, USSR
P. N. Lebedev Physical Institute of the Academy of Sciences of the USSR
Department of Theor. Physics, P. N. Lebedev Institute, 117924 Moscow, Russia
AN SSSR, Fizicheskii Institut, Moscow, USSR
P.N. Lebedev Physical Inst. of the Academy of Sciences, Moscow, Russia
P.N. Lebedev Physical Institute
P.N. Lebedev Physical Institute, 117924 Moscow, Russia
I. E. Tamm Theoretical Physics Division, P. N. Lebedev Physical Institute, 119991 Moscow, Russia
RAN, Fizicheskij Inst., Moscow, Russia
Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan; P. N. Lebedev Physical Institute, Leninskij Prospect, 53, 117924 Moscow, Russia
The Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510 of Space and Astronautical Science, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510, Japan; I. E. Tamm Department of Theoretical Physics, P. N. Lebedev Physical Institute, 119991 Moscow, Russia; Max-Planck-Institut für extraterrestrische Physik, Garching bei München, Germany of Space and Astronautical Science, 3-1-1 Sagamihara, Kanagawa 229-8510, Japan; I. E. Tamm Department of Theoretical Physics, P. N. Lebedev Physical Institute, 119991 Moscow, Russia; Max-Planck-Institut für extraterrestrische Physik, Garching bei München, Germany
A past capture event at Sagittarius A* inferred from the fluorescent X-ray emission of Sagittarius B clouds
An analysis of electron distributions in galaxy clusters by means of the flux ratio of iron lines FeXXV and XXVI
Annihilation Emission from the Galactic Black Hole
Book-Review - Astrophysics of Cosmic-Rays
Can Cosmic Rays BE Accelerated in Collapsing Molecular Clouds
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