activity
20132022
most citedOptically thick HI dominant in the local interstellar medium; an alternative interpretation to "dark gas"

81 citations · 361 across the 12 of their papers we have counts for

collaborators
Showing 2017Show all

4 papers · 1 filter

astro-ph.GA2017★ 5 cited

An Intermediate Velocity HI Cloud Falling to the Galactic Disk; Possible Evidence for Low Metallicity HI Gas Originated Outside the Galactic Disk

Yasuo Fukui, Masako Koga, Shohei Maruyama +6

We found that an intermediate velocity cloud (IVC) IVC 86-36 in HI 21 cm emission shows a head-tail distribution toward the Galactic plane with marked parallel filamentary streamer…

astro-ph.GA2017

Molecular and Atomic Clouds toward the Wolf-Rayet Nebula NGC 2359: Possible Evidence for Isolated High-Mass Star Formation Triggered by a Cloud-Cloud Collision

Hidetoshi Sano, Katsuhiro Hayashi, Rei Enokiya +17

NGC 2359 is an HII region located in the outer Galaxy that contains the isolated Wolf-Rayet (WR) star HD 56925. We present millimeter/submillimeter observations of CO( =…

astro-ph.HE2017★ 42 cited

A detailed study of the interstellar protons toward the TeV -ray SNR RX J0852.04622 (G266.21.2, Vela Jr.); a third case of the -rays and ISM spatial correspondence

Y. Fukui, H. Sano, J. Sato +18

We present a new analysis of the interstellar protons toward the TeV -ray SNR RX J0852.04622 (G266.21.2, Vela Jr.). We used the NANTEN2 CO( = 1-0) and ATCA & Par…

astro-ph.GA2017★ 27 cited

Synthetic Observations of 21cm HI Line Profiles from Inhomogeneous Turbulent Interstellar HI Gas with Magnetic Field

Yasuo Fukui, Takahiro Hayakawa, Tsuyoshi Inoue +5

We carried out synthetic observations of interstellar atomic hydrogen at 21cm wavelength by utilizing the magneto-hydrodynamical numerical simulations of the inhomogeneous turbulen…