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17 pages, 10 Figures, Invited paper at conference ``Cherenkov 2005'', Towards a Network of Atmospheric Cherenkov Detectors VII, at Ecole Polytechnique, Palaiseau (France), April 27-29, 2005; Editors: B. Degrange, G. Fontaine, pp. 233-245 (2006)
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The unstable isotope ^60 Fe, with a half-life of 2.6 million years, is produced primarily in supernova explosions. The observed presence of ^60 Fe in cosmic rays and its detection in deep-sea crusts and sediments suggest two possible scenarios: either ...
Xin-Yue Shi +2 more
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New Radio Observations of the Supernova Remnant CTA 1
We present new radio images of the supernova remnant (SNR) CTA 1 at 1420 and 408 MHz, and in the 21 cm line of H i observed with the Dominion Radio Astrophysical Observatory Synthesis Telescope and at 1420 MHz observed with the Effelsberg 100 m telescope.
Tam Do +5 more
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Energy of Tycho's supernova remnant is increasing with time. [PDF]
Barenblatt GI.
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A nearby long gamma-ray burst from a merger of compact objects. [PDF]
Troja E +23 more
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Anomalous cyclic in the neutrino oscillations. [PDF]
Aydiner E.
europepmc +1 more source
1051Ergs: The Evolution of Shell Supernova Remnants [PDF]
T. W. Jones +8 more
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The Sizes of OH (1720 MHz) Supernova Remnant Masers: MERLIN and Very Long Baseline Array Observations of IC 443 [PDF]
Ian M. Hoffman +4 more
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The role of the diffusive protons in the $\gamma$-ray emission of supernova remnant RX J1713.7-3946 --- a lepto-hadronic hybrid model [PDF]
Xiao Zhang, Yang Chen
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