Circinus X-1: survivor of a highly asymmetric supernova

Abstract

We have analyzed the kinematical parameters of Cir X-1 to constrain the nature of its companion star, the eccentricity of the binary and the pre-supernova parameter space. We argue that the companion is most likely to be a low-mass (< 2.0 M_sun) unevolved star and that the eccentricity of the orbit is 0.94 +/- 0.04. We have evaluated the dynamical effects of the supernova explosion and we find it must have been asymmetric. On average, we find that a kick of 740 km/s is needed to account for the recently measured radial velocity of +430 km/s (Johnston, Fender & Wu) for this extreme system. The corresponding minimum kick velocity is 500 km/s. This is the largest kick needed to explain the motion of any observed binary system. If Cir X-1 is associated with the supernova remnant G321.9-0.3 then we find a limiting minimum age of this remnant of 60000 yr. Furthermore, we predict that the companion star has lost 10% of its mass as a result of stripping and ablation from the impact of the supernova shell shortly after the explosion.

arXiv comment6 pages, 3 figues, 2 tables, accepted for publication in MNRAS

References in corpus (3)

• A New $\Sigma -D$ Relation and Its Application to the Galactic Supernova Remnant Distribution
• High resolution optical and infrared spectroscopic observations of Cir X-1
• An asymmetric arcsecond radio jet from Circinus X-1

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