activity
20092026
most citedFOREST Unbiased Galactic plane Imaging survey with the Nobeyama 45-m telescope (FUGIN) I: Project Overview and Initial Results

205 citations · 3.9k across the 163 of their papers we have counts for

collaborators
Showing 2022Show all

8 papers · 1 filter

astro-ph.HE2022★ 13 cited

New ASKAP Radio Supernova Remnants and Candidates in the Large Magellanic Cloud

Luke M. Bozzetto, Miroslav D. Filipović, H. Sano +34

We present a new Australian Square Kilometre Array Pathfinder (ASKAP) sample of 14 radio Supernova Remnant (SNR) candidates in the Large Magellanic Cloud (LMC). This new sample is…

astro-ph.GA2022★ 18 cited

Unraveling the observational signatures of cloud-cloud collision and hub-filament systems in W31

A. K. Maity, L. K. Dewangan, H. Sano +3

To understand the formation process of massive stars, we present a multi-scale and multi-wavelength study of the W31 complex hosting two extended HII regions (i.e., G10.30-0.15 (he…

astro-ph.HE2022★ 12 cited

Molecular and Atomic Clouds Associated with the Gamma-Ray Supernova Remnant Puppis A

M. Aruga, H. Sano, Y. Fukui +3

We have carried out a study of the interstellar medium (ISM) toward a shell-like supernova remnant SNR Puppis A by using the NANTEN CO and ATCA HI data. We synthesized a comprehens…

astro-ph.HE2022★ 17 cited

An Expanding Shell of Neutral Hydrogen Associated with SN 1006: Hints for the Single-Degenerate Origin and Faint Hadronic Gamma-Rays

H. Sano, H. Yamaguchi, M. Aruga +4

We report new HI observations of the Type Ia supernova remnant SN 1006 using the Australia Telescope Compact Array with an angular resolution of (2 pc at t…

astro-ph.HE2022★ 12 cited

Charge Exchange X-ray Emission Detected in Multiple Shells of Supernova Remnant G296.1-0.5

Yukiko Tanaka, Hiroyuki Uchida, Takaaki Tanaka +5

Recent high-resolution X-ray spectroscopy revealed possible presence of charge exchange (CX) X-ray emission in supernova remnants (SNRs). Although CX is expected to take place at o…

astro-ph.GA2022★ 20 cited

An ALMA study of the massive molecular clump N159W-North in the Large Magellanic Cloud: A possible gas flow penetrating one of the most massive protocluster systems in the Local Group

Kazuki Tokuda, Taisei Minami, Yasuo Fukui +18

Massive dense clumps in the Large Magellanic Cloud can be an important laboratory to explore the formation of populous clusters. We report multiscale ALMA observations of the N159W…