Multi-wavelength study of MGRO J2019+37

【摘要】 MGRO J2019+37,within the Cygnus region,is a bright extended source revealed by Milagro at 12-35 TeV.This source is almost as bright as the Crab Nebula in the northern sky,but is not confirmed by ARGO-YBJ around the TeV scale.Up to now,no obvious counterpart at low energy wavelengths has been found.Hence,MGRO J2019+37 is a rather mysterious object and its VHEγ-ray emission mechanism is worth investigating.In this paper,a brief summary of the multi-wavelength observations from radio toγ-rays is presented.All the available data from XMM-Newton and INTEGRAL at X-ray,and Fermi-LAT atγ-ray bands,are used to get constraints on its emission flux at low energy wavelengths.Then,its possible counterparts and the VHE emission mechanism are discussed.更多还原

【Abstract】 MGRO J2019+37, within the Cygnus region, is a bright extended source revealed by Milagro at 12-35 TeV. This source is almost as bright as the Crab Nebula in the northern sky, but is not confirmed by ARGO-YBJ around the TeV scale. Up to now, no obvious counterpart at low energy wavelengths has been found. Hence, MGRO J2019+37 is a rather mysterious object and its VHE γ-ray emission mechanism is worth investigating. In this paper,a brief summary of the multi-wavelength observations from radio to γ-rays is presented. All the available data from XMM-Newton and INTEGRAL at X-ray, and Fermi-LAT at γ-ray bands, are used to get constraints on its emission flux at low energy wavelengths. Then, its possible counterparts and the VHE emission mechanism are discussed.更多还原