SIMBAD references

2016MNRAS.456..347J - Mon. Not. R. Astron. Soc., 456, 347-355 (2016/February-2)

The nature of the companion star in Circinus X-1.

JOHNSTON H.M., SORIA R. and GIBSON J.

Abstract (from CDS):

We present optical spectra and images of the X-ray binary Circinus X-1. The optical light curve of Cir X-1 is strongly variable, changing in brightness by 1.2 mag in the space of four days. The shape of the light curve is consistent with that seen in the 1980s, when the X-ray and radio counterparts of the source were at least ten times as bright as they are currently. We detect strong, variable H α emission lines, consisting of multiple components which vary with orbital phase. We estimate the extinction to the source from the strength of the diffuse interstellar bands and the Balmer decrement; the two methods give AV = 7.6±0.6mag and AV > 9.1mag, respectively. The optical light curve can be modelled as arising from irradiation of the companion star by the central X-ray source, where a low-temperature star fills its Roche lobe in an orbit of moderate eccentricity (e ∼ 0.4). We suggest that the companion star is overluminous and underdense, due to the impact of the supernova which occurred less than 5000 yr ago.

Abstract Copyright: © 2015 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2015)

Journal keyword(s): binaries: spectroscopic - stars: individual: Cir X-1 - X-rays: binaries

Simbad objects: 5

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2021.01.15-17:24:28

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