activity
20172019
most citedFOREST Unbiased Galactic plane Imaging survey with the Nobeyama 45-m telescope (FUGIN) I: Project Overview and Initial Results

205 citations · 471 across the 8 of their papers we have counts for

collaborators

9 papers

astro-ph.HE201931 cited

Deep XMM-Newton Observations Reveal the Origin of Recombining Plasma in the Supernova Remnant W44

Hiromichi Okon, Takaaki Tanaka, Hiroyuki Uchida +8

Recent X-ray studies revealed over-ionized recombining plasmas (RPs) in a dozen mixed-morphology (MM) supernova remnants (SNRs). However, the physical process of the over-ionizatio…

astro-ph.GA201927 cited

ALMA Observations of Atomic Carbon [C I] () and Low- CO Lines in the Starburst Galaxy NGC 1808

Dragan Salak, Naomasa Nakai, Masumichi Seta +1

We present [C I] (), CO, CO, and CO () observations of the central region (radius 1 kpc) of the s…

astro-ph.GA201961 cited

CO Multi-line Imaging of Nearby Galaxies (COMING) IV. Overview of the Project

Kazuo Sorai, Nario Kuno, Kazuyuki Muraoka +36

Observations of the molecular gas in galaxies are vital to understanding the evolution and star-forming histories of galaxies. However, galaxies with molecular gas maps of their wh…

astro-ph.GA201960 cited

The JCMT BISTRO Survey: The Magnetic Field of the Barnard 1 Star-Forming Region

Simon Coudé, Pierre Bastien, Martin Houde +118

We present the POL-2 850 m linear polarization map of the Barnard 1 clump in the Perseus molecular cloud complex from the B-fields In STar-forming Region Observations (BISTRO) s…

astro-ph.GA201956 cited

The JCMT BISTRO Survey: The Magnetic Field In The Starless Core Ophiuchus C

Junhao Liu, Keping Qiu, David Berry +128

We report 850~m dust polarization observations of a low-mass (12 ) starless core in the Ophiuchus cloud, Ophiuchus C, made with the POL-2 instrument on the…

astro-ph.GA201926 cited

CO Multi-line Imaging of Nearby Galaxies (COMING): VI. Radial variations in star formation efficiency

Kazuyuki Muraoka, Kazuo Sorai, Yusuke Miyamoto +25

We examined radial variations in molecular-gas based star formation efficiency (SFE), which is defined as star formation rate per unit molecular gas mass, for 80 galaxies selected…