Browsing University of Galway Support Services by Subject "ism: supernova remnants"
Now showing items 1-5 of 5
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Discovery of tev gamma-ray emission toward supernova remnant snr g78.2+2.1
(IOP Publishing, 2013-05-29)We report the discovery of an unidentified, extended source of very-high-energy gamma-ray emission, VER J2019+407, within the radio shell of the supernova remnant SNR G78.2+2.1, using 21.4 hr of data taken by the VERITAS ... -
Discovery of very high energy γ-ray emission from the snr g54.1+0.3
(IOP Publishing, 2010-07-22)We report the discovery of very high energy (VHE) gamma-ray emission from the direction of the SNR G54.1+ 0.3 using the VERITAS ground-based gamma-ray observatory. The TeV signal has an overall significance of 6.8s and ... -
Investigating the tev morphology of mgro j1908+06 with veritas
(IOP Publishing, 2014-05-15)We report on deep observations of the extended TeV gamma-ray source MGRO J1908+06 made with the VERITAS very high energy gamma-ray observatory. Previously, the TeV emission has been attributed to the pulsar wind nebula ... -
Observations of the shell-type supernova remnant cassiopeia a at tev energies with veritas
(IOP Publishing, 2010-04-08)We report on observations of very high energy gamma rays from the shell-type supernova remnant (SNR) Cassiopeia A with the Very Energetic Radiation Imaging Telescope Array System stereoscopic array of four imaging atmospheric ... -
Towards an explanation for the 30 dor (lmc) honeycomb nebula - the impact of recent observations and spectral analysis
(Oxford University Press (OUP), 2010-08-18)The unique Honeycomb nebula, most likely a peculiar supernova remnant, lies in 30 Doradus in the Large Magellanic Cloud (LMC). Due to its proximity to SN1987A, it has been serendipitously and intentionally observed at many ...