Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
University of Tokyo
Laboratoire AIM Paris Saclay
CEA
ISO Science Operations Centre, Astrophysics Division, Space Science Department of ESA, Villafranca, P.O. Box 50727, E-28080 Madrid, Spain
Communications Research Laboratory, Nukui-kita 4-2-1, Koganei, Tokyo 184-8795, Japan
Institute for Cosmic Ray Research, The University of Tokyo, Tanashi, Tokyo 188, Japan
Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan
Institut d'Astrophysique Spatiale, Université Paris Sud, Bât. 121, 91405 Orsay Cedex, France; Service d'Astrophysique, CEA / DAPNIA, Saclay, France
Communications Research Laboratory
CRL, Japan
Department of Physics, Shinshu University, Nagano 390, Japan
Institut d'Astronomie Spatiale, Orsay, France
CEA-Saclay / DSM / Irfu / Service d'Astrophysique, France
Communications Research Laboratory, 4-2-1 Nukui-kitamachi, Koganei, Tokyo 184
Communications Research Laboratory, 4-2-1 Nukui-Kitamachi, Koganei, Tokyo 184
Kyushu U.
ICRR, U. of Tokyo
KEK
Department of Physics, Kyushu University, Fukuoka 812-8581, Japan
Department of Physics, Tohoku University, Sendai, 980-8578, Japan
Communications Research Lab.
$B \to X_s γ$ in minimal supersymmetric standard model with general flavor mixing
$μ\to e γ$ and $μ\to 3e$ Processes with Polarized Muon and Supersymmetric Grand Unified Theories
$μ\to e γ$ and $μ\to 3e$ processes with polarized muons and supersymmetric grand unified theories
155 Micron Continuum Emission from the Galactic Plane near L = 50 Degrees Observed by IRTS
A Deep and Ultra-deep ISOCAM Cosmological Survey through Gravitationally Lensing Clusters of Galaxies
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