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Gamma-ray binaries are among the most luminous very high-energy sources of the Galaxy. They consist of a normal star and a compact object, and their radiation is strongly variable and often periodic. Gamma-ray binaries also generate radio emission of non-thermal and sometimes extended nature, and X-rays, predominantly of non-thermal nature. These objects are strongly connected with other classes o ...
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 FINISHED 
This research project proposes to obtain the first unbiased survey on a large flux-limited sample of young stellar objects (YSOs) in 6 different molecular clouds. This study makes use of a huge dataset, namely various photometric maps from 0.6 μm up to 850 μm (including data from the Spitzer and the Herschel Space Telescope), and spectra (between 0.6 and 2.4 μm) of several YSOs in these clouds. Th ...
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