74 citations · 244 across the 8 of their papers we have counts for
8 papers
Current status and future plan of Osaka Prefecture University 1.85-m mm-submm telescope project
Atsushi Nishimura, Kazuki Tokuda, Ryohei Harada +25
We report the current status of the 1.85-m mm-submm telescope installed at the Nobeyama Radio Observatory (altitude 1400 m) and the future plan. The scientific goal is to reveal th…
Formation of High-Mass stars in an isolated environment in the Large Magellanic Cloud
Ryohei Harada, Toshikazu Onishi, Kazuki Tokuda +14
The aim of this study is to characterize the distribution and basic properties of the natal gas associated with high-mass young stellar objects (YSOs) in isolated environments in t…
An ALMA view of molecular filaments in the Large Magellanic Cloud II: An early stage of high-mass star formation embedded at colliding clouds in N159W-South
Kazuki Tokuda, Yasuo Fukui, Ryohei Harada +19
We have conducted ALMA CO isotopes and 1.3 mm continuum observations toward filamentary molecular clouds of the N159W-South region in the Large Magellanic Cloud with an angular res…
An ALMA view of molecular filaments in the Large Magellanic Cloud I: The formation of high-mass stars and pillars in the N159E-Papillon Nebula triggered by a cloud-cloud collision
Yasuo Fukui, Kazuki Tokuda, Kazuya Saigo +19
We present the ALMA observations of CO isotopes and 1.3 mm continuum emission toward the N159E-Papillon Nebula in the Large Magellanic Cloud (LMC). The spatial resolution is 0"25-0…
ALMA reveals molecular cloud N55 in the Large Magellanic Cloud as a site of massive star formation
N Naslim, K. Tokuda, T. Onishi +11
We present the molecular cloud properties of N55 in the Large Magellanic Cloud using CO(1-0) and CO(1-0) observations obtained with Atacama Large Millimeter Array. We…
ALMA observations of N83C in the early stage of star formation in the Small Magellanic Cloud
Kazuyuki Muraoka, Aya Homma, Toshikazu Onishi +14
We have performed Atacama Large Millimeter/submillimeter Array (ALMA) observations in CO(), CO(), CO(), CO(), CO($J=3…