activity
20102021
most citedSearch for photon line-like signatures from Dark Matter annihilations with H.E.S.S

251 citations · 952 across the 23 of their papers we have counts for

collaborators
Showing 2020Show all

5 papers · 1 filter

astro-ph.HE20203 cited

Arc-minute-scale studies of the interstellar gas towards HESSJ1804216: Still an unidentified TeV -ray source

K. Feijen, G. Rowell, S. Einecke +5

The Galactic TeV -ray source HESSJ1804216 is currently an unidentified source. In an attempt to unveil its origin, we present here the most detailed study of interstellar…

astro-ph.HE202023 cited

ALMA CO Observations of the Gamma-Ray Supernova Remnant RX J1713.7-3946: Discovery of Shocked Molecular Cloudlets and Filaments at 0.01 pc scales

H. Sano, T. Inoue, K. Tokuda +14

RX J1713.7-3946 is a unique core-collapse SNR that emits bright TeV gamma-rays and synchrotron X-rays caused by cosmic rays, in addition to interactions with interstellar gas cloud…

astro-ph.HE20202 cited

A supernova remnant associated with a nascent black hole low-mass X-ray binary

N. I. Maxted, A. J. Ruiter, K. Belczynski +2

Energy released when the core of a high-mass star collapses into a black hole often powers an explosion that creates a supernova remnant. Black holes have limited windows of observ…

astro-ph.GA2020

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…

astro-ph.GA20204 cited

Triggered high-mass star formation in the HII region W28A2: A cloud-cloud collision scenario

Katsuhiro Hayashi, Satoshi Yoshiike, Rei Enokiya +15

We report on a study of the high-mass star formation in the the HII region W28A2 by investigating the molecular clouds extended over ~5-10 pc from the exciting stars using the 12CO…