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Featured researches published by Tatsuji Kato.


Proceedings of The International Astronomical Union | 1989

VLA Polarization Observation of the Radio ARC at 15 GHZ

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

Observations of flat-spectrum QSOs at 43 GHz at NRO

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

The 10 GHz Log N — Log S Curve Obtained At NRO

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

LOG N - LOG S OF RADIO SOURCES AT 10 GHz WITH FLAT SPECTRA*

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

Extragalactic radio sources with very large Faraday rotation

Tatsuji Kato; Hiroto Tabara; Makoto Inoue; Ko Aizu


Publications of the Astronomical Society of Japan | 1995

Search for High Rotation Measures in Extragalactic Radio Sources I. Multi-Channel Observations at 10 GHz

Makoto Inoue; Hiroto Tabara; Tatsuji Kato; Ko Aizu


Publications of the Astronomical Society of Japan | 1993

Radio Polarization Observations of a Complete Sample of Core-Dominated Radio Sources

A. Okudaira; Hiroto Tabara; Tatsuji Kato; Makoto Inoue


Publications of the Astronomical Society of Japan | 1985

Two Highly Polarized Lobes near the Galactic Center

Masato Tsuboi; Makoto Inoue; Toshihiro Handa; Hiroto Tabara; Tatsuji Kato


Publications of the Astronomical Society of Japan | 1984

Observations of Weak Radio Sources with Flat or Inverted Spectra at 10 GHz

Hiroto Tabara; Tatsuji Kato; Makoto Inoue; Ko Aizu


Publications of the Astronomical Society of Japan | 1995

Galactic Center Arc-Polarized Plumes Complex at 43 GH_Z

Masato Tsuboi; Tetsuya Kawabata; Takashi Kasuga; Toshihiro Handa; Tatsuji Kato

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H. Tabara

Utsunomiya University

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