Radius and temperature evolution of the white dwarf in AS 296 during the 1988-1994 outburst

Details Radius and temperature evolution of the white dwarf in AS 296 during the 1988-1994 outburst Radius and temperature evolution of the white dwarf in AS 296 during the 1988-1994 outburst

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..797..615s&link_type=abstract

INTERACTING BINARIES: Accretion, Evolution, and Outcomes. AIP Conference Proceedings, Volume 797, pp. 615-618 (2005).

Physics

1

Symbiotic Stars, White Dwarfs, Stellar Dimensions, Cataclysmic Binaries, Symbiotic Stars, Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae, Radii

Scientific paper

Symbiotic stars undergo periodic TNR outbursts in which no mass is lost and the accreting white dwarf expands to the dimensions on a A-F giant/supergiant for several months or years before returning to the quiescent state. Several systems display eclipses that, coupled with an orbital solution, allow to determine the absolute values of the white dwarf mass, radius and temperature, and how them evolve during a outburst cycle. In this note we present preliminary results for the symbiotic system AS 296.

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