On the generation of relativistic particles in old novae

Details On the generation of relativistic particles in old novae On the generation of relativistic particles in old novae

Jul 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....59..289c&link_type=abstract

Astronomy and Astrophysics, vol. 59, no. 2, July 1977, p. 289-291.

Astronomy and Astrophysics

Astrophysics

6

Novae, Particle Acceleration, Radio Emission, Relativistic Particles, Nonthermal Radiation, Stellar Mass Ejection, Stellar Radiation, Stellar Spectrophotometry, Supernova Remnants, Thermal Emission

Scientific paper

The possibility is considered that relativistic particles may be generated by the interaction of nova ejecta with the ambient medium. The nature of this interaction is discussed for old nova shells, and possible acceleration mechanisms for the relativistic particles are noted, especially turbulence. Predictions regarding nonthermal radio emission from old novae are presented for V603 Aq1, DQ Her, CP Lac, GK Per, and RR Pic. It is concluded that the radio structure of nova remnants should be annular like those of various supernova remnants and that the radio fluxes should change appreciably on a time scale of years.

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