M. Fujimoto
Nagoya University
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Publication
Featured researches published by M. Fujimoto.
The Astrophysical Journal | 1983
Yoshiaki Sofue; M. Fujimoto
An analysis is made of Faraday rotation measures (RMs) of extragalactic radio sources. It is shown that a large-scale magnetic field in our Galaxy is oriented along the spiral arms. The field lines change their direction from one arm to the next across the neutral line in the interarm region. The loci of maximum field strength trace the spiral arms defined by H H II regions. Characteristic features of the RM distribution on the sky are well reproduced by a model in which the magnetic field is in a bisymmetric, two-armed logarithmic spiral configuration satisfying the flux conservation along the arm: the magnetic lines of force flow into the one half of the Galaxy in a spiral way and flow out from the diametrically opposite half.
The Astrophysical Journal | 1984
Toshiaki Takano; Yasuo Fukui; H. Ogawa; H. Takaba; Ryohei Kawabe; Y. Fujimoto; Koji Sugitani; M. Fujimoto
Publications of the Astronomical Society of Japan | 1974
Yoshiaki Sofue; M. Fujimoto
Publications of the Astronomical Society of Japan | 1990
Toshihiro Handa; N. Nakai; Yoshiaki Sofue; M. Hayashi; M. Fujimoto
The Astrophysical Journal | 1984
Ryohei Kawabe; H. Ogawa; Yasuo Fukui; Toshiaki Takano; H. Takaba; Y. Fujimoto; Koji Sugitani; M. Fujimoto
Publications of the Astronomical Society of Japan | 1983
Toshiaki Takano; H. Ogawa; Taichi Kato; M. Fujimoto; Y. Fujimoto; Yasuo Fukui; Yoshikazu Hayashi; K. Kawabata; Ryohei Kawabe; Yoshiaki Sofue
Astronomy and Astrophysics | 1976
M. Fujimoto; Yoshiaki Sofue
Symposium - International Astronomical Union | 1990
M. Fujimoto; Yoshiaki Sofue
Archive | 1988
T. Handal; Yoshiaki Sofue; N. Nakai; M. Hayashi; M. Fujimoto
International astronomical union. Symposium. 115 | 1987
Toshihiro Handa; Yoshiaki Sofue; N. Nakai; M. Fujimoto; Mitsuru R. Hayashi
