スポンサーリンク
National Astronomical Observatory Of Japan Tokyo | 論文
- Optical and Near-Infrared Photometric Observation during the Superoutburst of the WZ Sge-Type Dwarf Nova, V455 Andromedae
- Direct Observation of the Extended Molecular Atmosphere of o Ceti by Differential Spectral Imaging with an Adaptive Optics System
- Suzaku Observation of HCG 62 : Temperature, Abundance, and Extended Hard X-Ray Emission Profiles
- In-orbit timing calibration of the hard X-ray detector on board Suzaku
- Multiple-Component Analysis of the Time-Resolved Spectra of GRB 041006 : A Clue to the Nature of the Underlying Soft Component of GRBs
- Spectral evolution of GRB 060904A observed with swift and Suzaku : Possibility of inefficient electron acceleration
- The Suzaku-Swift Joint Observation of the Early X-Ray Afterglow of GRB060105(Chapter 1. Gamma Ray Bursts, Cosmic Rays and Neutrino, The Extreme Universe in the Suzaku Era)
- A multiband study of the optically dark GRB 051028
- Global Radiation-Magnetohydrodynamic Simulations of Black-Hole Accretion Flow and Outflow : Unified Model of Three States
- The X-Ray Observatory Suzaku
- Discovery of Molecular Loop 3 in the Galactic Center : Evidence for a Positive-Velocity Magnetically Floated Loop towards L=355°-359°
- Similarity between the Molecular Loops in the Galactic Center and the Solar Chromospheric Arch Filaments
- A Peculiar Jet and Arc of Molecular Gas toward the Rich and Young Stellar Cluster Westerlund 2 and a TeV Gamma Ray Source
- Catalogue of ^CO(J = 1-0) and ^CO(J = 1-0) Molecular Clouds in the Carina Flare Supershell
- Aligned Molecular Clouds towards SS 433 and L = 348°.5 : Possible Evidence for a Galactic "Vapor Trail" Created by a Relativistic Jet
- Discovery of Interacting Molecular Gas toward the TeV Gamma-Ray Peak of the SNR G 347.3-0.5
- A Large-Scale Study of H^CO^+and C^O (J = 1-0) in Orion B
- The Most Massive C^O Molecular Complex in Centaurus and Star Formation Therein
- Detection of Eight Molecular Supershells in the Southern Milky Way with NANTEN
- A CO Survey of the LMC with NANTEN : III. Formation of Stellar Clusters and Evolution of Molecular Clouds