Tatsuji Kato
Utsunomiya University
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Featured researches published by Tatsuji Kato.
Proceedings of The International Astronomical Union | 1989
M. Inoue; E. Fomalont; M. Tsuboi; Farhad Yusef-Zadeh; Mark R. Morris; H. Tabara; Tatsuji Kato
Polarization measurements of the radio Arc were made with the VLA at 15 GHz. High frequency polarimetry made with high spatial resolution minimizes Faraday depolarization and reveals polarized filaments which correspond to the predominant filaments of the radio Arc. We notice a peculiar linear feature in the polarization map (“thorns”) which suggests the presence of a second magnetic field system. The total intensity maps show no evidence for an interaction between the two field systems, so the thorns may be foreground magnetized structures. However, if the two magnetic field systems do interact, it would allow a model in which the acceleration of relativistic particles takes place at their intersection. The accelerated particles would flow toward both ends of the radio Arc, and account for the intrinsic polarization observed along the entire length of the system. Thermal electrons responsible for the Faraday depolarization occuring at longer wavelengths may be supplied by the interaction of the streams of relativistic particles with relatively dense, ambient thermal clouds.
Vistas in Astronomy | 1988
Ko Aizu; Makoto Inoue; Hiroto Tabara; Tatsuji Kato
Abstract Using the 45-m telescope at NRO we measured flux densities at 43 GHz of 115 flat-spectrum radio sources selected from 5 GHz catalogues. A preliminary log N ∼ log S curve is obtained. A simple model interpretation of the curve is given.
Symposium - International Astronomical Union | 1987
Ko Aizu; Makoto Inoue; Hiroto Tabara; Tatsuji Kato
Using 45-m radio-telescope at NRO, we obtained log N — log S curves at 10 GHz for flat- and steep-spectrum sources separately. A simple model-fitting of evolution is given
Astrophysics and Space Science | 1986
Ko Aizu; Hiroto Tabara; Tatsuji Kato; Makoto Inoue
A log N — log S relation at 10 GHz is constructed for sources with the flat spectra α ≤ 0.5 (flux density S ∞ ν −α) from observations at NRO, MPIfR and others. Based on the source distribution on log (Luminosity) ~ volume plane we obtain an epoch-depending luminosity function, which explains the above relation.
Nature | 1987
Tatsuji Kato; Hiroto Tabara; Makoto Inoue; Ko Aizu
Publications of the Astronomical Society of Japan | 1995
Makoto Inoue; Hiroto Tabara; Tatsuji Kato; Ko Aizu
Publications of the Astronomical Society of Japan | 1993
A. Okudaira; Hiroto Tabara; Tatsuji Kato; Makoto Inoue
Publications of the Astronomical Society of Japan | 1985
Masato Tsuboi; Makoto Inoue; Toshihiro Handa; Hiroto Tabara; Tatsuji Kato
Publications of the Astronomical Society of Japan | 1984
Hiroto Tabara; Tatsuji Kato; Makoto Inoue; Ko Aizu
Publications of the Astronomical Society of Japan | 1995
Masato Tsuboi; Tetsuya Kawabata; Takashi Kasuga; Toshihiro Handa; Tatsuji Kato