Orbital periods of cataclysmic variables identified by the SDSS - VI. The 4.5-h period eclipsing system SDSS J100658.40+233724.4

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Table 6:

Eclipsing cataclysmic variables for which masses and radii of one or both components has been measured accurately and precisely.
$\begin{displaymath}{\begin{tabular}{l c r@{~$\pm$~}l r@{~$\pm$~}l r@{~$\pm$~}l r... ...0.11 & \multicolumn{2}{c}{0.90} & 16 \\ \hline \end{tabular}} \end{displaymath}$ Those secondary radii without errorbars are not available from the original reference so have instead been calculated assuming Roche geometry. References: (1) Ribeiro et al. (2007); (2) Copperwheat et al. in preparation; (3) Gänsicke et al. (2000); (4) Thorstensen (2000); (5) Feline et al. (2005); (6) Marsh et al. (1990); (7) Long & Gilliland (1999); (8) Naylor et al. (2005); (9) Echevarría et al. (2007); (10) Horne et al. (1993); (11) Wood et al. (2005); (12) Fiedler et al. (1997); (13) Baptista et al. (2000); (14) Baptista & Catalán (2001); (15) Thoroughgood et al. (2005); (16) Thoroughgood et al. (2004).

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