The early blast wave of the 2010 explosion of U Scorpii

TL;DR

This study uses 3D hydrodynamic simulations to analyze the early blast wave of U Scorpii's 2010 outburst, revealing how initial conditions influence blast morphology and X-ray emissions.

Contribution

It provides the first detailed 3D simulation of the initial 18 hours of U Scorpii's outburst, highlighting the effects of system geometry and initial parameters on blast evolution.

Findings

Blast wave is collimated with bipolar structures.

X-ray luminosity depends on ejecta mass and circumstellar density.

Ejecta mass likely not exceeding 10^{-7} solar masses.

Abstract

Three-dimensional hydrodynamic simulations exploring the first 18 hours of the 2010 January 28 outburst of the recurrent nova U Scorpii have been performed. Special emphasis was placed on capturing the enormous range in spatial scales in the blast. The pre-explosion system conditions included the secondary star and a flared accretion disk. These conditions can have a profound influence on the evolving blast wave. The blast itself is shadowed by the secondary star, which itself gives rise to a low-temperature bow-shock. The accretion disk is completely destroyed in the explosion. A model with a disk gas density of 10^{15} cm^{-3} produced a blast wave that is collimated and with clear bipolar structures, including a bipolar X-ray emitting shell. The degree of collimation depends on the initial mass of ejecta, energy of explosion, and circumstellar gas density distribution. It is most pronounced for a model with the lowest explosion energy (10^{43} erg) and mass of ejecta (10^{-8} M_{\odot}). The X-ray luminosities of three of six models computed are close to, but consistent with, an upper limit to the early blast X-ray emission obtained by the Swift satellite, the X-ray luminosity being larger for higher circumstellar gas density and higher ejecta mass. The latter consideration, together with estimates of the blast energy from previous outbursts, suggests that the mass of ejecta in the 2010 outburst was not larger than 10^{-7} M_{\odot}.