スポンサーリンク
Department Of Astronomical Science Graduate University For Advanced Studies Nobeyama Radio Observato | 論文
- CO J = 3-2 Emission from the "Water Fountain" Sources IRAS 16342-3814 and IRAS 18286-0959
- SiO and H_2O Maser Observations of Red Supergiants in Star Clusters Embedded in the Galactic Disk
- Japanese VLBI Network Mapping of SiO v = 3 J = 1-0 Maser Emission in W Hydrae
- Near-IR Observations of IRAS Sources with SiO Masers at the Inner Galactic Bulge
- SiO Maser Survey of Cold IRAS Sources
- SiO Maser Survey toward the Inner Galactic Disk : 40°≦l≦70° and |b|≦10°
- SiO Maser Survey of Southern IRAS Sources
- Observations of Stellar Maser Sources with No IRAS Counterpart
- Study of the Bipolar Nebula IRAS 19312+1950 : II. Circumstellar Chemistry
- SiO Maser Survey of IRAS Sources in the Inner Galactic Disk
- SiO Maser Survey of the Large-Amplitude Variables in the Galactic Center
- Study of the Bipolar Nebula IRAS 19312+1950 : I. Mapping Observations
- Near-Infrared Observations of the IRAS/SiO Sources in the Galactic Bulge : a Large Scale Distribution
- Detection of SiO Masers from the Large-Amplitude Variables in the Galactic Nuclear Disk
- Observations of SiO Maser Sources within a Few Parsec from the Galactic Center
- Period Measurement of AGB Stars in the Outer Galactic Disk
- Detections of SiO and H_2O Masers in the Bipolar Nebula IRAS 19312+1950
- SiO Maser Spectra of V407 Cygni after the 2010 March Nova Outburst
- Extremely Strong ^CO J=3→2 Line in the "Water Fountain" IRAS 16342-3814 : Evidence for the Hot-Bottom Burning
- Pilot VLBI Survey of SiO υ=3 J=1→0 Maser Emission around Evolved Stars