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2010

AGILE detection of GeV gamma-ray emission from the SNR W28

Giuliani, A., Tavani, M., Bulgarelli, A. et al.

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Supernova remnants (SNRs) are believed to be the main sources of Galactic cosmic rays.

Molecular clouds associated with SNRs can produce gamma-ray emission through the interaction of accelerated particles with the concentrated gas.
The middle aged SNR W28, for its associated system of dense molecular clouds, provides an excellent opportunity to test this hypothesis.
We present the AGILE/GRID observations of SNR W28, and compare them with observations at other wavelengths (TeV and 12CO J=1-->0 molecular line emission).

AGILE detection of GeV gamma-ray emission from the SNR W28 · Around

Built on

Mem. S.A.It. Sup
Giuliani, A. et al. (2004) · 2004
Earlier work this paper cites.
ASP Conference Series
Mizuno, A. and Fukui, Y. (2004) · 2004
Earlier work this paper cites.

Similar

Nucl. Instr. and Meth. A
Giuliani, A. et al. (2006) · 2006
Cited alongside, same era.
Nucl. Instr. and Meth. A
Tavani, M. et al. (2008) · 2008
Cited alongside, same era.

Then

Green, D. A. 2009, Bulletin of the Astronomical Society of India, 37, 45
2009
Later among the works it cites.
In preparation
Chen, A. et al. (2010) · 2010
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