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
Publicado:	2013
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:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v557_n_p_Castelletti 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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