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Oxford University Press (OUP), Monthly Notices of the Royal Astronomical Society, 1(403), p. 398-404

DOI: 10.1111/j.1365-2966.2009.16128.x

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High speed photometry of faint cataclysmic variables - VI. Car2, V1040 Cen, Hα 075648, IL Nor (Nova Nor 1893), HS Pup (Nova Pup 1963), SDSS , CSS and CSS

Journal article published in 2010 by Patrick A. Woudt ORCID, Brian Warner
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

We have observed 8 faint cataclysmic variable stars photometrically. The nova-like Car2 was extensively sampled but showed little variability. V1040 Cen was observed near the end of a dwarf nova outburst and possessed dwarf nova and quasi-periodic oscillations. Ha 075648 has strong large amplitude flickering and a possible orbital modulation at 3.49 h. The correct identification for the nova remnant IL Nor (Nova Nor 1893) has been established. HS Pup (Nova Pup 1963) has a possible orbital period of 3.244 h. SDSS J2048-06 is a low mass transfer dwarf nova that in quiescence shows slow variations at 7.67 h (though poorly sampled with our observations) and an orbital modulation at 87.26 min. The dwarf nova CSS 081419-005022 has an orbital period of 1.796 h and the eclipsing dwarf nova CSS 112634-100210 has an orbital period of 1.8581 h. ; Comment: 7 pages, 15 figures. Accepted for publication in MNRAS