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