T. Shimoikura

activity

20002026

most citedRevealing the physical properties of molecular gas in Orion with a large scale survey in J=2-1 lines of 12CO, 13CO and C18O

132 citations · 1.1k across the 46 of their papers we have counts for

collaborators

Showing 2017Show all

3 papers · 1 filter

astro-ph.GA2017★ 4 cited

Correlation of gas dynamics and dust in the evolved filament G82.65-02.00

M. Saajasto, M. Juvela, K. Dobashi +12

The combination of line and continuum observations can provide vital insights to the formation and fragmentation of filaments and the initial conditions for star formation. We have…

astro-ph.GA2017★ 19 cited

Observations of Cyanopolyynes toward Four High-Mass Star-Forming Regions Containing Hot Cores

Kotomi Taniguchi, Masao Saito, Tomoya Hirota +7

We carried out line survey observations at the 26-30 GHz band toward the four high-mass star-forming regions containing hot cores, G10.30-0.15, G12.89+0.49, G16.86-2.16, and G28.28…

astro-ph.GA2017★ 19 cited

Wide-Field $^{12}$ CO ( $J = 2 - 1$ ) and $^{13}$ CO ( $J = 2 - 1$ ) Observations toward the Aquila Rift and Serpens Molecular Cloud Complexes. I. Molecular Clouds and Their Physical Properties

Fumitaka Nakamura, Kazuhito Dobashi, Tomomi Shimoikura +2

We present results of wide-field $^{12}$ CO ( $J = 2 - 1$ ) and $^{13}$ CO ( $J = 2 - 1$ ) observations toward the Aquila Rift and Serpens molecular cloud complexes (25$^\circ < l < 33^\…

Correlation of gas dynamics and dust in the evolved filament G82.65-02.00

Observations of Cyanopolyynes toward Four High-Mass Star-Forming Regions Containing Hot Cores

Wide-Field 12CO (J=2−1) and 13CO (J=2−1) Observations toward the Aquila Rift and Serpens Molecular Cloud Complexes. I. Molecular Clouds and Their Physical Properties

Wide-Field $^{12}$ CO ( $J = 2 - 1$ ) and $^{13}$ CO ( $J = 2 - 1$ ) Observations toward the Aquila Rift and Serpens Molecular Cloud Complexes. I. Molecular Clouds and Their Physical Properties