102 citations · 1.1k across the 89 of their papers we have counts for
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Astrochemical Properties of Planck Cold Clumps
Ken'ichi Tatematsu, Tie Liu, Satoshi Ohashi +25
We observed thirteen Planck cold clumps with the James Clerk Maxwell Telescope/SCUBA-2 and with the Nobeyama 45 m radio telescope. The NH distribution obtained with the Nob…
Characterizing the properties of cluster precursors in the MALT90 survey
Yanett Contreras, Jill M. Rathborne, Andres Guzman +4
In the Milky Way there are thousands of stellar clusters each harboring from a hundred to a million stars. Although clusters are common, the initial conditions of cluster formation…
Dense core properties in the Infrared Dark cloud G14.225-0.506 revealed by ALMA
Satoshi Ohashi, Patricio Sanhueza, Huei-Ru Vivien Chen +5
We have performed a dense core survey toward the Infrared Dark Cloud G14.225-0.506 at 3 mm continuum emission with the Atacama Large Millimeter/Submillimeter Array (ALMA). This sur…
Detection of a turbulent gas component associated with a starless core with subthermal turbulence in the Orion A cloud
Satoshi Ohashi, Ken'ichi Tatematsu, Patricio Sanhueza +4
We report the detection of a wing component in NH emission toward the starless core TUKH122 with subthermal turbulence in the Orion A cloud. This NH core is suggested to be…
Linking Dense Gas from the Milky Way to External Galaxies
Ian W. Stephens, James M. Jackson, J. Scott Whitaker +5
In a survey of 65 galaxies, Gao & Solomon (2004) found a tight linear relation between the infrared luminosity (, a proxy for the star formation rate) and the HCN(1-0)…