279 citations · 1.1k across the 23 of their papers we have counts for
23 papers
ALMA Observations of Supernova Remnant N49 in the Large Magellanic Cloud. II. Non-LTE Analysis of Shock-heated Molecular Clouds
H. Sano, Y. Yamane, J. Th. van Loon +28
We present the first compelling evidence of shock-heated molecular clouds associated with the supernova remnant (SNR) N49 in the Large Magellanic Cloud (LMC). Using CO( =…
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…
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…
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…
The Long Tails of the Pegasus-Pisces Arch Intermediate Velocity Cloud
R. L. Shelton, M. E. Williams, M. C. Parker +3
We present hydrodynamic simulations of the Pegasus-Pisces (PP Arch), an intermediate velocity cloud in our Galaxy. The PP Arch, also known as IVC 86-36, is unique among intermediat…
Discovery of a Wind-Blown Bubble Associated with the Supernova Remnant G346.6-0.2: A Hint for the Origin of Recombining Plasma
H. Sano, H. Suzuki, K. K. Nobukawa +3
We report on CO and HI studies of the mixed-morphology supernova remnant (SNR) G346.60.2. We find a wind-blown bubble along the radio continuum shell with an expansion velocity…