Radio emission from supernova remnants

The explosion of a supernova releases almost instantaneously about 10$$^{51}$$51 ergs of mechanic energy, changing irreversibly the physical and chemical properties of large regions in the galaxies. The stellar ejecta, the nebula resulting from the powerful shock waves, and sometimes a compact stell...

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Detalles Bibliográficos
Autores principales: Dubner, G., Giacani, E.
Formato: JOUR
Materias:
ISM: cosmic rays
ISM: supernova remnants
Radiation mechanisms: non-thermal
Radio continuum: ISM
Balloons
Cosmology
Galaxies
Radio astronomy
Shock waves
Stars
Electromagnetic spectra
Physical and chemical properties
Physical characteristics
Polarization properties
Radiation mechanisms: non thermal
Supernovae
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_09354956_v23_n1_p_Dubner
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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