Morphological and spectral properties of the W51 region measured with the MAGIC telescopes
Morphological and spectral properties of the W51 region measured with the MAGIC telescopes
The W51 complex hosts the supernova remnant W51C which is known to interact with the molecular clouds in the star forming region W51B. In addition, a possible pulsar wind nebula CXO J192318.5+140305 was found likely associated with the supernova remnant. Gamma-ray emission from this region was discovered by Fermi/LAT (between …