activity
20082026
most citedThe Quiescent Intracluster Medium in the Core of the Perseus Cluster

500 citations · 1k across the 31 of their papers we have counts for

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Showing 2018Show all

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astro-ph.HE2018

Suzaku X-ray observations of the mixed-morphology supernova remnant CTB 1

Miho Katsuragawa, Shinya Nakashima, Hideaki Matsumura +6

We present an X-ray study of the mixed-morphology supernova remnant CTB 1 (G116.9+0.2) observed with Suzaku. The 0.6-2.0 keV spectra in the northeast breakout region of CTB 1 are w…

astro-ph.HE2018

Detection of polarized gamma-ray emission from the Crab nebula with Hitomi Soft Gamma-ray Detector

Hitomi Collaboration, Felix Aharonian, Hiroki Akamatsu +191

We present the results from the Hitomi Soft Gamma-ray Detector (SGD) observation of the Crab nebula. The main part of SGD is a Compton camera, which in addition to being a spectrom…

astro-ph.HE2018

Chandrasekhar and sub-Chandrasekhar models for the X-ray emission of Type Ia supernova remnants (I): Bulk properties

Héctor Martínez-Rodríguez, Carles Badenes, Shiu-Hang Lee +9

Type Ia supernovae originate from the explosion of carbon-oxygen white dwarfs in binary systems, but the exact nature of their progenitors remains elusive. The bulk properties of T…

astro-ph.HE2018

Shock acceleration of electrons and synchrotron emission from the dynamical ejecta of neutron star mergers

Shiu-Hang Lee, Keiichi Maeda, Norita Kawanaka

Neutron star mergers (NSMs) eject energetic sub-relativistic dynamical ejecta into the circumbinary media. As analogous to supernovae and supernova remnants, the NSM dynamical ejec…

astro-ph.HE2018

Hitomi X-ray Observation of the Pulsar Wind Nebula G21.50.9

Hitomi Collaboration, Felix Aharonian, Hiroki Akamatsu +194

We present results from the Hitomi X-ray observation of a young composite-type supernova remnant (SNR) G21.50.9, whose emission is dominated by the pulsar wind nebula (PWN) cont…

astro-ph.HE2018

Evidence for GeV Cosmic Rays from White Dwarfs in the Local Cosmic Ray Spectra and in the Gamma-ray Emissivity of the Inner Galaxy

Tuneyoshi Kamae, Shiu-hang Lee, Kazuo Makishima +2

Recent observations found that electrons are accelerated to 10 GeV and emit synchrotron hard X-rays in two magnetic white dwarfs (WDs), also known as cataclysmic variables (C…