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Nobeyama Radio Observatory, National Astronomical Observatory | 論文
- FTS Measurements of Submillimeter-Wave Atmospheric Opacity at Pampa la Bola : III. Water Vapor, Liquid Water, and 183GHz Water Vapor Line Opacities
- 2 Millimeter Dust around NGC 7538-IRS 1, 2, and 3 : I. Unfilled Structure of Dust Cloud
- The Virgo High-Resolution CO Survey : I. CO Atlas
- The Spatial Distributions of SO and N_2H^+ in Taurus Molecular Cloud-1(TMC-1)
- The Ortho-to-Para Ratio and the Chemical Properties of C_3H_2 in Dark Cloud Cores
- Distribution and Dynamics of Molecular Gas in the Galaxy M51. III. Kinematics of Molecular Gas
- CO (J = 1-0) Observation of the cD Galaxy of AWM 7:Constraints on the Evaporation of Molecular Gas
- Variation of Molecular Gas Properties Across the Spiral Arms in IC 342 : Large-Scale ^CO (1-0) Emission
- A Spectral-Line Survey Observation of IRC +10216 between 28 and 50 GH_z
- FTS Measurements of Submillimeter-Wave Atmospheric Opacity at Pampa la Bola II: Supra-Terahertz Windows and Model Fitting
- Two-Millimeter Observations of the Starburst Galaxy M82
- SiO Maser Spectra of V407 Cygni after the 2010 March Nova Outburst
- Initial Results from Nobeyama Molecular Gas Observations of Distant Bright Galaxies
- Extremely Strong ^CO J=3→2 Line in the "Water Fountain" IRAS 16342-3814 : Evidence for the Hot-Bottom Burning
- Global destabilization due to localized reconnection : A mechanism for coronal
- Global destabilization due to localized reconnection: A mechanism for coronal mass ejections