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ALMA twenty-six arcmin2 survey of GOODS-S at one millimeter (ASAGAO): Millimeter properties of stellar mass selected galaxies
DOI: 10.1093/pasj/psaa057 Bibcode: 2020PASJ...72...69Y

Ouchi, Masami; Fujimoto, Seiji; Tamura, Yoichi +19 more

We make use of the ALMA twenty-Six Arcmin2 survey of GOODS-S At One-millimeter (ASAGAO), deep 1.2 mm continuum observations of a 26-arcmin2 region in the Great Observatories Origins Deep Survey-South (GOODS-S) obtained with Atacama Large Millimeter/sub-millimeter Array (ALMA), to probe dust-enshrouded star formation in K-band…

2020 Publications of the Astronomical Society of Japan
Gaia Herschel eHST 10
HCN 3-2 survey towards a sample of local galaxies
DOI: 10.1093/pasj/psaa025 Bibcode: 2020PASJ...72...41L

Fang, Min; Li, Shanghuo; Wang, Junzhi +4 more

We present observations of HCN 3-2 emissions towards 37 local galaxies using the 10 m Submillimeter Telescope. HCN 3-2 emission is detected in 23 galaxies. The correlation of infrared luminosity (LIR) and the luminosity of HCN 3-2 line emission measured in our sample is fitted with a slope of 1.11 and correlation coefficient of 0.91, wh…

2020 Publications of the Astronomical Society of Japan
Herschel 7
A systematic study of Galactic infrared bubbles along the Galactic plane with AKARI and Herschel. II. Spatial distributions of dust components around the bubbles
DOI: 10.1093/pasj/psz123 Bibcode: 2020PASJ...72....5H

Oyabu, Shinki; Kaneda, Hidehiro; Ishihara, Daisuke +7 more

Galactic infrared (IR) bubbles, which can be seen as shell-like structures at mid-IR wavelengths, are known to possess massive stars within their shell boundaries. In our previous study (Hanaoka, 2019, PASJ, 71, 6), we expanded the research area to the whole Galactic plane (0° ≤ l ≤ 360°, |b| ≤ 5°) and studied systematic differences in the shell m…

2020 Publications of the Astronomical Society of Japan
AKARI Herschel 3