Abstract
view Abstract Citations (46) References (29) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS The evolution of nonthermal supernova remnants. II. Can radio supernovae become plerions ? Bandiera, R. ; Pacini, F. ; Salvati, M. Abstract The authors discuss the evolution of pulsar-driven supernova remnants. It is shown that the early stages closely resemble the phenomenon of radio supernovae and that one can establish a direct evolutionary link between the two classes of objects. Light curves are obtained in the radio and the X-ray ranges under simple assumptions about the injected spectrum. The derived relations between surface brightness and diameter, both at low and at high frequencies, are compared with the observational data. Publication: The Astrophysical Journal Pub Date: October 1984 DOI: 10.1086/162484 Bibcode: 1984ApJ...285..134B Keywords: Nonthermal Radiation; Radio Sources (Astronomy); Stellar Evolution; Supernova Remnants; Brightness; Diameters; Light Curve; Pulsars; X Ray Sources; Astrophysics full text sources ADS | data products SIMBAD (8) NED (5) Related Materials (1) Erratum: 1985ApJ...291..394B
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