most citedMolecular Clouds associated with the Type Ia SNR N103B in the Large Magellanic Cloud

31 citations · 120 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2018★ 20 cited

ALMA CO Observations of Supernova Remnant N63A in the Large Magellanic Cloud: Discovery of Dense Molecular Clouds Embedded within Shock-Ionized and Photoionized Nebulae

H. Sano, H. Matsumura, T. Nagaya +19

We carried out new CO( = 1-0, 3-2) observations of a N63A supernova remnant (SNR) from the LMC using ALMA and ASTE. We find three giant molecular clouds toward the northe…

astro-ph.HE2018★ 17 cited

ALMA observations of supernova remnant N49 in the LMC: I. Discovery of CO clumps associated with X-ray and radio continuum shells

Y. Yamane, H. Sano, J. Th. van Loon +24

N49 (LHA 120-N49) is a bright X-ray supernova remnant (SNR) in the Large Magellanic Cloud. We present new CO( = 1-0, 3-2), HI, and 1.4 GHz radio-continuum observations of…

astro-ph.GA2018★ 31 cited

Molecular Clouds associated with the Type Ia SNR N103B in the Large Magellanic Cloud

H. Sano, Y. Yamane, K. Tokuda +18

N103B is a Type Ia supernova remnant (SNR) in the Large Magellanic Cloud (LMC). We carried out new CO( = 3-2) and CO( = 1-0) observations using ASTE and ALMA. W…

astro-ph.HE2018★ 22 cited

Possible Evidence for Cosmic-Ray Acceleration in the Type Ia SNR RCW 86: Spatial Correlation between TeV Gamma rays and Interstellar Atomic Protons

H. Sano, G. Rowell, E. M. Reynoso +13

We present a detailed morphological study of TeV gamma rays, synchrotron radiation, and interstellar gas in the young Type Ia supernova remnant (SNR) RCW 86. We find that the inter…

astro-ph.GA2017★ 30 cited

Discovery of molecular and atomic clouds associated with the gamma-ray supernova remnant Kesteven 79

M. Kuriki, H. Sano, N. Kuno +21

We carried out CO( = 1-0) observations of the Galactic gamma-ray supernova remnant (SNR) Kesteven 79 using the Nobeyama Radio Observatory 45 m radio telescope, which has…