Cosmic rays in the surroundings of SNR G35.6-0.4
HESS J1858+020 is a TeV gamma-ray source that was reported to have no clearly catalogued counterpart at any wavelength. However, it has been recently proposed that this source is indirectly associated with the radio source, re-identified as a supernova remnant (SNR), G35.6-0.4. The latter has been f...
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| Autores principales: | Torres, D.F., Li, H., Chen, Y., Cillis, A., Caliandro, A.G., Rodríguez-Marrero, A.Y. |
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| Formato: | JOUR |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00358711_v417_n4_p3072_Torres |
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