A hadronic scenario for HESS J1818-154

Aims. G15.4+0.1 is a faint supernova remnant (SNR) that has recently been associated with the γ-ray source HESS J1818-154. We investigate a hadronic scenario for the production of the γ-ray emission. Methods. Molecular 13CO (J = 1-0) taken from the Galactic Ring Survey (GRS) and neutral hydrogen (HI...

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Detalles Bibliográficos
Autores principales: Castelletti, G., Supan, L., Dubner, G., Joshi, B.C., Surnis, M.P.
Formato: JOUR
Materias:
Gamma rays: ISM
ISM: individual objects: J1818-154
ISM: supernova remnants
Radio continuum: ISM
Galactic plane surveys
Gamma rays: isms
Giant metrewave radio telescopes
High-energy emissions
ISM: individual objects
Molecular materials
Clouds
Gamma rays
Stars
Estimation
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00046361_v557_n_p_Castelletti
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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