... Cancri

Tables 1 and 2 are only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.125.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/398/239

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... date

Note that another dwarf M-type eclipsing binary was reported and analysed by Maceroni & Rucinski (1997). The system, which was discovered by the OGLE survey, is very faint ( $V \approx 18.3$) and the physical properties of the components are currently not well constrained. Moreover, the light curve solution indicates strongly distorted components with the primary possibly filling its Roche lobe.

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... components

Note, however, that the sum of fractional radii is extremely well determined because it depends strongly on the total duration of the eclipses.

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... distance

Note that there is a weak dependence of the bolometric correction on the temperature, so these expressions are only valid for temperatures not too far off from those in Table 4.

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