Discovery Of Complex Tev Emission Towards The Cyg Ob1 Region And Other Observations Of Complex Regions With Veritas

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We report the discovery of a complex region of emission above 650 GeV towards of the Cyg OB1 association using the VERITAS ground-based TeV observatory. This emission is positionally compatible with the brightest part of MGRO J2019+37 seen above 12 TeV, and which has been interpreted as the nebula of the bright radio and gamma-ray pulsar PSR J2021+3651. Instead, VERITAS resolves the MGRO emission into a complex gamma-ray emission region, likely composed of multiple sources, and distinct from nearby SNR CTB 87. A broadband study of this region with the available archival data in radio, X-rays and GeV gamma-rays has been performed and compared to these new TeV maps. We will report about the MW results of another complex region in which VERITAS has detected TeV emission, in the direction of the Cep OB2.

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