SiO Maser Survey of Southern IRAS Sources
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概要
- 論文の詳細を見る
- Astronomical Society of Japanの論文
- 2001-04-25
著者
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NAKASHIMA Jun-ichi
Department of Physics, University of Hong Kong
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DEGUCHI Shuji
Nobeyama Radio Observatory, National Astronomical Observatory
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Deguchi Shuji
Nobeyama Radio Observatory National Astronomical Observatory
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Deguchi Shuji
Nobeyama Radio Observatory
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BALASUBRAMANYAM Ramesh
School of Physics, University of New South Wales
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Nakashima Jun-ichi
Department Of Astronomical Science Graduate University For Advanced Studies Nobeyama Radio Observato
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Nakashima Jun-ichi
Department Of Astronomical Science The Graduate University For Advanced Studies
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Balasubramanyam Ramesh
School Of Physics University Of New South Wales
関連論文
- CO J = 3-2 Emission from the "Water Fountain" Sources IRAS 16342-3814 and IRAS 18286-0959
- A Search for Water Masers in the Saturnian System
- SiO Maser Survey off the Galactic Plane : A Signature of Streaming Motion
- 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
- Apparent Double SiO Maser Sources
- Near-Infrared Observations of IRAS Sources With SiO Masers in the Direction of the Near End of the Galactic Bar
- Infrared Identification of SiO Maser Sources toward the Sgr B2 Molecular Cloud
- Water-Vapor Maser Survey for Active Galactic Nuclei : A Megamaser in NGC 6926
- Detection of SiO Maser Emission in V838 Mon
- SiO Maser Survey of Cold IRAS Sources
- SiO Maser Survey toward the Inner Galactic Disk : 40°≦l≦70° and |b|≦10°
- A Measurement of Proper Motions of SiO Maser Sources in the Galactic Center with the VLBA
- VLBA Observation of SiO Masers in the M Giant IRC -10414
- Japanese VLBI Network Observations of SiO Masers in the M-Type Giant IRC-10414
- JVN Observation of H_2O Masers around the Evolved Star IRAS 22480+6002
- Clustering of Meter-Wave Luminous Objects toward Monoceros
- Kashima 34-m Water Maser Survey of Late-Type Stars
- Wave Optics in Gravitational Lensing
- SiO Maser Survey in the Galactic Center Region with a Multi-Beam Receiver
- SiO Maser Survey of Southern IRAS Sources
- An SiO Maser Search off the Galactic Plane
- SiO Maser Survey of the Inner Bar of the Galactic Bulge
- Observations of Stellar Maser Sources with No IRAS Counterpart
- SiO Maser Sources toward Globular Clusters
- SiO Maser Sources toward Globular Clusters
- 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
- SiO Maser Survey of Cold IRAS Sources
- 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
- HOCO^+ toward the Galactic Center
- Time Variation of SiO Masers in VX Sagittarii over an Optically Quiescent Phase
- Detections of SiO and H_2O Masers in the Bipolar Nebula IRAS 19312+1950
- SiO Masers in Stars in the Inner and Outer Galactic Disk
- Evidence for a Dense, Cold Screen towards IRAS 18507+0121
- SiO Maser Survey of the Galactic Bulge IRAS Sources IV. Observational Properties of SiO Masers
- Kinematics of Red Variables in the Solar Neighborhood I. Basic Data Obtained by an SiO Maser Survey
- SiO Maser Spectra of V407 Cygni after the 2010 March Nova Outburst
- Maser Emission toward the Infrared Dark Cloud G359.94+0.17 Seen in Silhouette against the Galactic Center
- 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
- Elective Cesarean Section at 37 Weeks Is Associated with the Higher Risk of Neonatal Complications