A J-band detection of the donor star in the dwarf nova OY Carinae, and an optical detection of its `iron curtain'

TL;DR

This study uses time-resolved spectroscopy to confirm the donor star's radial velocity in OY Carinae and detects the 'iron curtain' in optical wavelengths, providing new insights into the system's accretion disc dynamics.

Contribution

First optical detection of the 'iron curtain' in OY Carinae and validation of photometric binary parameters through spectroscopic measurements.

Findings

Donor star's radial velocity K2 = 470.0 +/- 2.7 km/s matches predictions.

Detection of Fe I and Fe II lines indicating the 'iron curtain' in the accretion disc.

Evidence of significant radial motion in the outer disc, up to 90 km/s.

Abstract

Purely photometric models can be used to determine the binary parameters of eclipsing cataclysmic variables with a high degree of precision. However, the photometric method relies on a number of assumptions, and to date there have been very few independent checks of this method in the literature. We present time-resolved spectroscopy of the P=90.9 min eclipsing cataclysmic variable OY Carinae obtained with X-shooter on the VLT, in which we detect the donor star from K I lines in the J-band. We measure the radial velocity amplitude of the donor star K2 = 470.0 +/- 2.7 km/s, consistent with predictions based upon the photometric method (470 +/- 7 km/s). Additionally, the spectra obtained in the UVB arm of X-shooter show a series of Fe I and Fe II lines with a phase and velocity consistent with an origin in the accretion disc. This is the first unambiguous detection at optical wavelengths of the `iron curtain' of disc material which has been previously reported to veil the white dwarf in this system. The velocities of these lines do not track the white dwarf, reflecting a distortion of the outer disc that we see also in Doppler images. This is evidence for considerable radial motion in the outer disk, at up to 90 km/s towards and away from the white dwarf.