From the 1 of 2.3k papers with an AI index.
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- The University of TokyoJP780 papers
- Kyoto UniversityJP454 papers
- Centre National de la Recherche ScientifiqueFR396 papers
- The University of OsakaJP392 papers
- Tokyo Institute of TechnologyJP376 papers
- High Energy Accelerator Research OrganizationJP372 papers
- National Astronomical Observatory of JapanJP318 papers
- Chinese Academy of SciencesCN315 papers
- Tokyo Metropolitan UniversityJP314 papers
- University of Science and Technology of ChinaCN311 papers
- The University of MelbourneAU306 papers
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120 papers · 1 filter
Triggered O star formation in M20 via cloud-cloud collision: Comparisons between high-resolution CO observations and simulations
Kazufumi Torii, Yusuke Hattori, Keisuke Hasegawa +9
High-mass star formation is one of the top-priority issues in astrophysics. Recent observational studies are revealing that cloud-cloud collisions may play a role in high-mass star…
HCN hyperfine ratio analysis of massive molecular clumps
W. J. Schap, P. J. Barnes, A. Ordonez +3
We report a new analysis protocol for HCN hyperfine data, based on the PYSPECKIT package, and results of using this new protocol to analyse a sample area of seven massive molecular…
An analysis of star formation with Herschel in the Hi-GAL Survey. II. The tips of the Galactic bar
M. Veneziani, E. Schisano, D. Elia +20
We present the physical and evolutionary properties of prestellar and protostellar clumps in the Herschel Infrared GALactic plane survey (Hi-GAL) in two large areas centered in the…
The Exoplanet Mass-Ratio Function from the MOA-II Survey: Discovery of a Break and Likely Peak at a Neptune Mass
D. Suzuki, D. P. Bennett, T. Sumi +26
We report the results of the statistical analysis of planetary signals discovered in MOA-II microlensing survey alert system events from 2007 to 2012. We determine the survey sensi…
Faint source star planetary microlensing: the discovery of the cold gas giant planet OGLE-2014-BLG-0676Lb
N. J. Rattenbury, D. P. Bennett, T. Sumi +85
We report the discovery of a planet --- OGLE-2014-BLG-0676Lb --- via gravitational microlensing. Observations for the lensing event were made by the MOA, OGLE, Wise, RoboNET/LCOGT,…
A statistical study of giant molecular clouds traced by CO, CO, CS, and CHOH in the disk of NGC 1068 based on ALMA observations
Tomoka Tosaki, Kotaro Kohno, Nanase Harada +7
We present (98 pc) resolution ALMA observations of CO(=1-0), CO(=1-0), CS(=2-1) and CHOH(=-) molecular lines in the central (…