An interacting molecular cloud scenario for production of gamma-rays and neutrinos from MAGIC J1835-069, and MAGIC J1837-073

Abstract Recently the MAGIC telescope observed three TeV gamma-ray extended sources in galactic plane neighborhood of radio SNR G24.7+0.6. Among them, PWN HESS J1837-069 was detected earlier by observatory during its first survey. The other two sources, J1835-069 and J1837-073 are for time at such high energies. Here we shall show that gamma-rays from G24.7+0.6 can be explained terms hadronic interactions PWN/SNR accelerated cosmic rays with ambient matter. We further demonstrate interpreted through runaway cosmic-rays molecular cloud location J1837-073. No association has been found between or J1837-069. have examined maximum energy attainable cosmic-ray particles G24.7+0.6/ possibility their detection future telescopes. study neutrino emissions stated suggests should IceCube Gen-2 a few years observation.