SNR G24.7+0.6 is a 9.5 kyrs radio and γ-ray supernova remnant evolving in a dense medium. In the GeV regime, SNR G24.7+0.6 (3FHL J1834.1-0706e/FGES J1834.1-0706...
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PublicaciónDiscovery of TeV γ-ray emission from the neighbourhood of the supernova remnant G24.7+0.6 by MAGIC
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PublicaciónDiscovery of TeV γ-ray emission from the pulsar wind nebula 3C 58 by MAGIC
Context. The pulsar wind nebula (PWN) 3C 58 is one of the historical very high-energy (VHE; E> 100 GeV) γ-ray source candidates. It is energized by one of the...
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PublicaciónDiscovery of Very High Energy Gamma Radiation from IC 443 with the MAGIC Telescope
We report the detection of a new source of very high energy (VHE; Eγ>=100 GeV) γ-ray emission located close to the Galactic plane, MAGIC J0616+225, which is...
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CharlaDusty supernovae running the thermodynamics of the matter reinserted by young stellar clusters
Following the observational and theoretical evidence that points at core collapse supernovae as major producers of dust, we calculate the hydrodynamics of the...
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PublicaciónErratum: A cut-off in the TeV gamma-ray spectrum of the SNR Cassiopeia A
The paper `A cut-off in the TeV gamma-ray spectrum of the SNR Cassiopeia A' was originally published in 472(3), 2956-2962.
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PublicaciónEvidence for high velocity gas in giant H II regions
Spectroscopy of selected areas of the two Giant H II Regions (GHR) NGC 5471 and NGC 604 shows convincing evidence for the existence of ionized gas at high...
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PublicaciónEvolution of supernova remnants inside preexisting wind-driven cavities
The evolution of supernova remnants in preexisting cavities is examined by means of 1D and 2D numerical studies of the phenomenon and the fragmentation of...
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CharlaGamma-ray bursts as a tool to unveil obscured star-forming galaxies
Long Gamma-Ray Bursts are flashes of high-energy radiation and are linked to the death of massive stars. I will first summarize the main aspects of GRB...
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PublicaciónHidden supernova remnants in the Large Magellanic Cloud H II complex N44
We have obtained ROSAT PSPC observations of N44, one of the largest H II complexes in the Large Magellanic Cloud. The X-ray emission mostly fails within the...