Time resolved spectroscopy and photometry of three little known bright cataclysmic variables: LS IV -08${}^{\mathrm{o}}$ 3, HQ Monocerotis and ST Chamaeleontis

Abstract

As part of a project to better characterize comparatively bright but so far little studied cataclysmic variables in the southern hemisphere, we have obtained spectroscopic and photometric data of the nova-like variables LS IV -08${}^{\mathrm{o}}$ 3 and HQ Mon, and of the Z Cam type dwarf nova ST Cha. The spectra of all systems are as expected for their respective types. We derive improved orbital ephemeris of LS IV -08${}^{\mathrm{o}}$ 3 and map its accretion disk in the light of the H$\alpha$ emission using Doppler tomography. We find that the emission has a two component origin, arising in the outer parts of the accretion disk and possibly on the illuminated face of the secondary star. The light curve of LS IV -08${}^{\mathrm{o}}$ 3 exhibits a low level of flickering and indications for a modulation on the orbital period. Spectroscopy of HQ Mon suggests an orbital period of $\approx$5.15 hours which is incompatible with previous (uncertain) estimates. The light curves show the typical low scale flickering of UX UMa type nova-like systems, superposed upon variations on longer time scales. During one night a modulation with a period of $\approx$41 min is observed, visible for at least 4 hours. However, it does not repeat itself in other nights. A spectroscopic orbital period of $\approx$5.5 hours is derived for ST Cha. A previously suspected period of 6.8 hours (or alternatively 9.6 hours), based on historical photographic photometry is incompatible with the spectroscopic period. Moreover, we show that our new as well as previous photometry does not contain evidence for the quoted photometric period.

References in corpus (8)

• The Fourth US Naval Observatory CCD Astrograph Catalog (UCAC4)
• Achieving better than 1 minute accuracy in the Heliocentric and Barycentric Julian Dates
• Catalogue of cataclysmic binaries, low-mass X-ray binaries and related objects (Seventh edition)
• The Evolution of Cataclysmic Variables as Revealed by their Donor Stars
• Post-common-envelope binaries from SDSS. XI: The white dwarf mass distributions of CVs and pre-CVs
• Three in one go: consequential angular momentum loss can solve major problems of CV evolution
• Photometry of the long period dwarf nova MU Centauri
• A New, Bright, Short-Period, Emission Line Binary in Ophiuchus

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