S. Ohashi

activity

20132026

μ

m dark High-mass clumps in Early Stages (ASHES). I. Pilot Survey: Clump Fragmentation

207 citations · 1.9k across the 45 of their papers we have counts for

collaborators

Showing 2015Show all

2 papers · 1 filter

astro-ph.GA2015★ 9 cited

Chemical evolution of the HC3N and N2H+ molecules in dense cores of the Vela C giant molecular cloud complex

Satoshi Ohashi, Ken'ichi Tatematsu, Kosuke Fujii +5

We have observed the HC3N (J=10-9) and N2H+ (J=1-0) lines toward the Vela C molecular clouds with the Mopra 22 m telescope to study chemical characteristics of dense cores. The int…

astro-ph.SR2015★ 114 cited

The two molecular clouds in RCW 38; evidence for formation of the youngest super star cluster in the Milky Way triggered by cloud-cloud collision

Y. Fukui, K. Torii, A. Ohama +13

We present distributions of two molecular clouds having velocities of 2 km s $^{- 1}$ and 14 km s $^{- 1}$ toward RCW 38, the youngest super star cluster in the Milky Way, in the $^{12…