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
Autores principales: Supan, L., Castelletti, G., Joshi, B.C., Surnis, M.P., Supanitsky, D.
Formato: JOUR
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: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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