activity
20062022
most citedThe Formation and Destruction of Molecular Clouds and Galactic Star Formation

253 citations · 3.6k across the 61 of their papers we have counts for

collaborators

61 papers

astro-ph.HE2022★ 2 cited

Study of the effect of turbulent interstellar mediums on young supernova remnant morphology

Gabriel Rigon, Tsuyoshi Inoue

Context. Supernova remnants (SNR) are one of the main sources of galactic cosmic rays acceleration. This acceleration, believed to happen at the blast wave front, leads to an energ…

astro-ph.GA2022★ 41 cited

B-fields in Star-Forming Region Observations (BISTRO): Magnetic Fields in the Filamentary Structures of Serpens Main

Woojin Kwon, Kate Pattle, Sarah Sadavoy +149

We present 850 m polarimetric observations toward the Serpens Main molecular cloud obtained using the POL-2 polarimeter on the James Clerk Maxwell Telescope (JCMT) as part of th…

astro-ph.GA2021★ 23 cited

The JCMT BISTRO Survey: An 850/450m Polarization Study of NGC 2071IR in OrionB

A-Ran Lyo, Jongsoo Kim, Sarah Sadavoy +143

We present the results of simultaneous 450 m and 850 m polarization observations toward the massive star forming region NGC 2071IR, a target of the BISTRO (B-fields in Star-F…

astro-ph.HE2021★ 27 cited

Direct Numerical Simulations of Cosmic-ray Acceleration at Dense Circumstellar Medium: Magnetic Field Amplification by Bell Instability and Maximum Energy

Tsuyoshi Inoue, Alexandre Marcowith, Gwenael Giacinti +2

Galactic cosmic rays are believed to be accelerated at supernova remnants. However, whether supernova remnants can be Pevatrons is still very unclear. In this work we argue that Pe…

astro-ph.HE2021★ 28 cited

Pursuing the origin of the gamma rays in RX J1713.73946 quantifying the hadronic and leptonic components

Yasuo Fukui, Hidetoshi Sano, Yumiko Yamane +5

We analyzed the TeV gamma-ray image of a supernova remnant RX J1713.73946 (RX J1713) through a comparison with the interstellar medium (ISM) and the non-thermal X-rays. The gamm…

astro-ph.GA2021★ 10 cited

Giant Molecular Cloud Formation at the Interface of Colliding Supershells in the Large Magellanic Cloud

Kosuke Fujii, Norikazu Mizuno, J. R. Dawson +8

We investigate the Hi envelope of the young, massive GMCs in the star-forming regions N48 and N49, which are located within the high column density Hi ridge between two kpc-scale s…