23 citations · 38 across the 3 of their papers we have counts for
7 papers
ALMA CO Observations of Gamma-Ray Supernova Remnant N132D in the Large Magellanic Cloud: Possible Evidence for Shocked Molecular Clouds Illuminated by Cosmic-Ray Protons
H. Sano, P. P. Plucinsky, A. Bamba +23
N132D is the brightest gamma-ray supernova remnant (SNR) in the Large Magellanic Cloud (LMC). We carried out CO( = 1-0, 3-2) observations toward the SNR using the Atacama…
Diagnosing Cosmic Ray Modified Shocks with H α Polarimetry
Jiro Shimoda, J. Martin Laming
A novel diagnostic of cosmic-ray modified shocks by polarimetry of H emissions is suggested. In a cosmic-ray modified shock, the pressure of cosmic rays is sufficiently high co…
ALMA Polarimetry of AT2018cow
K. Y. Huang, J. Shimoda, Y. Urata +7
We present the first radio polarimetric observations of a fast-rising blue optical transient, AT2018cow. Two epochs of polarimetry with additional coincident photometry were perfor…
Radiative transfer of hydrogen lines from supernova remnant shock waves: contributions of 2s-state hydrogen atoms
Jiro Shimoda, J. Martin Laming
Radiative transfer in hydrogen lines in supernova remnant (SNR) shock waves is studied taking into account the population of the hydrogen atom 2s-state. Measurements of Balmer line…
Discovery of Kolmogorov-like Magnetic Energy Spectrum in Tycho's Supernova Remnant by Two-point Correlations of Synchrotron Intensity
Jiro Shimoda, Takuya Akahori, A. Lazarian +2
The spectral slope of the magnetic energy in supernova remnants (SNRs) can be obtained by analysis of spatial two-point correlation functions of synchrotron intensities. This metho…
Polarized Balmer Line Emission from Supernova Remnant Shock Waves Efficiently Accelerating Cosmic Rays
Jiro Shimoda, Yutaka Ohira, Ryo Yamazaki +2
Linearly polarized Balmer line emissions from supernova remnant shocks are studied taking into account the energy loss of the shock owing to the production of nonthermal particles.…