RS Ophiuchi: Thermonuclear Explosion or Disc Instability?

TL;DR

This paper proposes that RS Ophiuchi's outbursts are caused by thermal-viscous instabilities in an irradiated accretion disc, challenging the standard thermonuclear explosion model and explaining observed jets and outburst characteristics.

Contribution

It introduces a disc instability model for RS Oph's outbursts, addressing inconsistencies in the thermonuclear explosion paradigm.

Findings

Disc instability model explains jets and outburst features.

Standard thermonuclear model faces difficulties with observed jets.

Large accretion disc size fits the instability scenario.

Abstract

Sokoloski et al (2008) have recently reported evidence that the recurrent nova RS Ophiuchi produced a pair of highly collimated radio jets within days of its 2006 outburst. This suggests that an accretion disc must be present during the outburst. However in the standard picture of recurrent novae as thermonuclear events, any such disc must be expelled from the white dwarf vicinity, as the nuclear energy yield greatly exceeds its binding energy. We suggest instead that the outbursts of RS Oph are thermal--viscous instabilities in a disc irradiated by the central accreting white dwarf. The distinctive feature of RS Oph is the very large size of its accretion disc. Given this, it fits naturally into a consistent picture of systems with unstable accretion discs. This picture explains the presence and speed of the jets, the brightness and duration of the outburst, and its rise time and linear decay, as well as the faintness of the quiescence. By contrast, the hitherto standard picture of recurrent thermonuclear explosions has a number of severe difficulties. These include the presence of jets, the faintness of quiescence, and the fact the the accretion disc must be unstable unless it is far smaller than any reasonable estimate.