Radio continuum and near-infrared study of the MGRO J2019+37region***

Authors :: Paredes, J. M.
Martí, J.
Ishwara-Chandra, C. H.
Sánchez-Sutil, J. R.
Muñoz-Arjonilla, A. J.
Moldón, J.
Peracaula, M.
Luque-Escamilla, P. L.
Zabalza, V.
Bosch-Ramon, V.
Bordas, P.
Romero, G. E.
Ribó, M.
Paredes, J. M.
Martí, J.
Ishwara-Chandra, C. H.
Sánchez-Sutil, J. R.
Muñoz-Arjonilla, A. J.
Moldón, J.
Peracaula, M.
Luque-Escamilla, P. L.
Zabalza, V.
Bosch-Ramon, V.
Bordas, P.
Romero, G. E.
Ribó, M.
Source :: Astronomy and Astrophysics; November 2009, Vol. 507 Issue: 1 p241-250, 10p
Publication Year :: 2009
Abstract: Context. MGRO J2019+37is an unidentified extended source of very high energy gamma-rays originally reported by the Milagro Collaboration as the brightest TeV source in the Cygnus region. Its extended emission could be powered by either a single or several sources. The GeV pulsar AGL J2020.5+3653, discovered by AGILE and associated with PSR J2021+3651, could contribute to the emission from MGRO J2019+37.

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