A complete radio study of SNR G15.4+0.1 from new GMRT observations

Aims. The supernova remnant (SNR) G15.4+0.1 is considered to be the possible counterpart of the γ-ray source HESS J1818-154. With the goal of getting a complete view of this remnant and understanding the nature of the γ-ray flux, we conducted a detailed radio study that includes the search for pulsa...

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Detalles Bibliográficos
Publicado:	2015
Materias:	Gamma rays: ISM ISM: individual objects: SNR G15.4+0.1 ISM: supernova remnants Radio continuum: ISM Astronomy Pulsars Radio telescopes Supernovae Far infrared wavelengths Galactic plane surveys Gamma rays: isms Giant metrewave radio telescopes ISM: individual objects Spectral energy distribution Gamma rays
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v576_n_p_Supan http://hdl.handle.net/20.500.12110/paper_00046361_v576_n_p_Supan
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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