A new study of the supernova remnant G344.7-0.1 located in the vicinity of the unidentified TeV source HESS J1702-420

Context. The identification of counterparts of dark gamma-ray sources adds greatly to our understanding of their underlying astrophysical processes. Aims. We investigate the physical properties of the supernova remnant (SNR) G344.7-0.1, to clarify whether it hosts a pulsar wind nebula (PWN), and the...

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Detalles Bibliográficos
Autores principales: Giacani, E., Smith, M.J.S., Dubner, G., Loiseau, N.
Formato: JOUR
Materias:
Gamma rays: ISM
ISM: individual objects: G344.7 - 0.1
ISM: supernova remnants
X-rays: individuals: HESS J1702-420
Blast waves
Compressed gas
Dense materials
Gamma ray sources
High resolution
Interstellar mediums
ISM: individual objects
New study
Pulsar wind nebulae
Radio images
Second generation
Stellar wind
Supernova remnants
Turbulent environments
X ray radiation
XMM-Newton
Spectrum analysis
Stars
Tellurium compounds
X rays
Gamma rays
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00046361_v531_n_p_Giacani
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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