Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
University of Tokyo
UTokyo
University of Tokyo, Japan
Institute of Astronomy, University of Tokyo
Faculty of Education, Wakayama University, Wakayama 640-8510
Central Rotation Curves of Spiral Galaxies
Compatibility of the CO and HI Linewidths Considering the Gas Distribution and Rotation Curves
Distance Determination of Galaxies in the Deep Universe Using LMSA
Distance Measurement of Galaxies to Redshift of 0.1 using the CO-Line Tully-Fisher Relation
Effects of Galaxy Interaction on the Tully-Fisher Relation: CO vs HI Linewidths
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