Kazufumi Torii
0000-0003-2450-1611
自然科学研究機構国立天文台
75 papers found
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High-Mass Star Formation Triggered by Collision Between Co Filaments in N159 West in the Large Magellanic Cloud
Cloud–cloud Collision as a Trigger of the High-Mass Star Formation: A Molecular Line Study in Rcw 120
Isolating signatures of major cloud–cloud collisions using position–velocity diagrams
A DETAILED STUDY OF NON-THERMAL X-Ray PROPERTIES AND INTERSTELLAR GAS TOWARD THE γ-Ray SUPERNOVA REMNANT RX J1713.7–3946
Optically Thick H I Dominant in the Local Interstellar Medium: An Alternative Interpretation to “dark Gas”
${\Rm H\,\scriptsize{I}}$, CO, ANDPLANCK/IRASDUST PROPERTIES IN THE HIGH LATITUDE CLOUD COMPLEX, MBM 53, 54, 55 AND HLCG 92 – 35. POSSIBLE EVIDENCE FOR AN OPTICALLY THICK ${\Rm H\,\scriptsize{I}}$ ENVELOPE AROUND THE CO CLOUDS
Planck2013 results. XIII. Galactic CO emission
Mapping the Milky Way bulge at high resolution: the 3D dust extinction, CO, and X factor maps
INTERSTELLAR PROTONS IN THE TeV γ-Ray SNR HESS J1731-347: POSSIBLE EVIDENCE FOR THE COEXISTENCE OF HADRONIC AND LEPTONIC γ-Rays
The JET AND ARC MOLECULAR CLOUDS TOWARD WESTERLUND 2, RCW 49, AND HESS J1023–575;12CO AND13CO (J= 2-1 andJ= 1-0) OBSERVATIONS WITH NANTEN2 AND MOPRA TELESCOPE
Detailed molecular observations toward the Double Helix Nebula
Molecular Clouds Toward the Super Star Cluster Ngc 3603; Possible Evidence for a Cloud-Cloud Collision in Triggering the Cluster Formation
NON-THERMAL X-Rays AND INTERSTELLAR GAS TOWARD THE γ-Ray SUPERNOVA REMNANT RX J1713.7–3946: EVIDENCE FOR X-Ray ENHANCEMENT AROUND CO AND H I CLUMPS
Large-scale mapping of the massive star-forming region RCW38 in the [CII] and PAH emission
The NEUTRAL INTERSTELLAR GAS TOWARD SNR W44: CANDIDATES FOR TARGET PROTONS IN HADRONIC γ-Ray PRODUCTION IN a MIDDLE-AGED SUPERNOVA REMNANT
Discovery of possible molecular counterparts to the infrared Double Helix Nebula in the galactic center
Processing of Polycyclic Aromatic Hydrocarbons in Molecular-Loop Regions near the Galactic Center Revealed by AKARI
Molecular and Atomic Gas toward HESS J1745−303 in the Galactic Center: Further Support for the Hadronic Scenario
A DETAILED STUDY OF THE MOLECULAR AND ATOMIC GAS TOWARD THE γ-Ray SUPERNOVA REMNANT RX J1713.7–3946: SPATIAL TeV γ-Ray AND INTERSTELLAR MEDIUM GAS CORRESPONDENCE
Stochastic Acceleration of Cosmic Rays in the Central Molecular Zone of the Galaxy: Fig. 1.
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