Physics
Scientist
Инсmumуm ме∂uко-бuолоzuческuх nроблем
Universität Würzburg, Würzburg, Germany
1=Centro de Radioastronomía y Astrofísica, UNAM, 2=Korea Astronomy and Space Science Institute, 3=Astrophysikalisches Institut Potsdam
Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, PA
Hebrew U.
Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain
1. Instituto de Astronomía, Universidad Nacional Autónoma de México, Ensenada; 2. Centro de Radioastronomía y Astrofísica, Universidad Nacional Autónoma de México, Morelia; 3. Japan Aerospace Exploration Agency, Tokyo, Japan
Instituto de Fisica da USP, SP, Brazil
Centro Atomico Bariloche, Argentina
1-Dept. Physics, Univ. Patras, Greece. 2-Dept. Physics & Astronomy, Univ. Manchester, England. 3-NRAL, Univ. Manchester, England.
University of Hertfordshire, Hertfordshire, UK
Nion Co. Seattle, WA, U.S.A
Dipartimento di Fisica, Universita di Milano-Bicocca, Milano
1- EPFL Switzerland, 2- Cardiff Univ. UK, 3- Univ. Zurich Switzerland, 4- Univ. Liege Belgium
1 - Jodrell Bank Centre for Astrophysics, University of Manchester, 2 - Dept. of Physics, University of West Virginia, 3 - Max Planck Institut fur Radioastronomie, Bonn, 4 - National Radio Astronomy Observatory, Green Bank
Max-Planck-Institut für Astronomie, Heidelberg. Germany
University of Texas at Brownsville, TX
1 - Jodrell Bank Centre for Astrophysics, University of Manchester, 2 - Max Planck Institut fuer Radioastronomie, 3 - Dept. of Physics, University of West Virginia, 4 - National Radio Astronomy Observatory, Green Bank
Universidad Autonoma de Madrid
ESO / ECF, Garching, Germany
University of Birmingham
Dpto. Física Atómica, Molecular y Nuclear, Facultad de Física, Universidad Complutense de Madrid, Ciudad Universitaria, Madrid
P.N. Lebedev Physics Institute, Moscow, Russia
Istituto Nazionale di Fisica Nucleare-Sez. Torino Italy
1 - Jodrell Bank Centre for Astr
$^1S_0$ superfluid phase--transition in neutron matter with realistic nuclear potentials and modern many--body theories
$Ω_0 <1$ From Inflation
Результаты и перспективы микроБиологиче&
A 100-kpc inverse Compton X-ray halo around 4C60.07 at z=3.79
A 2.14 ms Candidate Optical Pulsar in SN1987A
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