The OmegaWhite survey for short-period variable stars – III: follow-up photometric and spectroscopic observations

• Published in: Monthly notices of the Royal Astronomical Society Vol. 465; no. 1; p. 434
• Main Authors: Macfarlane, S A, Woudt, P A, Groot, P J, Ramsay, G, Toma, R, Motsoaledi, M, Crause, L A, Gilbank, D G, O'Donoghue, D, Potter, S B, Sickafoose, A A, van Gend, C, Worters, H L
• Format: Journal Article
• Language: English
• Published: London Oxford University Press 11-02-2017
• Subjects: Aerial surveys; Amplitudes; Astronomy; Light; Photometry; Space telescopes; Spectra; Spectroscopic telescopes; Spectroscopy; Star & galaxy formation; Stars; Africa
• ISSN: 0035-8711; 1365-2966
• DOI: 10.1093/mnras/stw2704

We present photometric and spectroscopic follow-up observations of short-period variables discovered in the OmegaWhite survey, a wide-field high-cadence g-band synoptic survey targeting the Galactic Plane. We have used fast photometry on the SAAO 1.0- and 1.9-m telescopes to obtain light curves of 27 variables, and use these results to validate the period and amplitude estimates from the OmegaWhite processing pipeline. Furthermore, 57 sources (44 unique, 13 with new light curves) were selected for spectroscopic follow-up using either the SAAO 1.9-m telescope or the Southern African Large Telescope. We find that many of these variables have spectra which are consistent with being d Scuti-type pulsating stars. At higher amplitudes, we detect four possible pulsating white dwarf/subdwarf sources and an eclipsing cataclysmic variable. Due to their rarity, these targets are ideal candidates for detailed follow-up studies. From spectroscopy, we confirm the symbiotic binary star nature of two variables identified as such in the SIMBAD database. We also report what could possibly be the first detection of the 'Bump Cepheid' phenomena in a d Scuti star, with OW J175848.21-271653.7 showing a pronounced 22 per cent amplitude dip lasting 3 min during each pulsational cycle peak. However, the precise nature of this target is still uncertain as it exhibits the spectral features of a B-type star.