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E. Farrell edited section4.tex
about 10 years ago
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\paragraph{}
The authors find that the number of observed eclipsing binaries
scales \emph{scales directly with the input
frequency frequency} of short-period orbits. For example, although typically less than 1\% of eclipsing FG systems show 1.5 mag eclipses, the ratio at the shortest periods is closer to 20\%. The situation is more complex for higher mass sytems although the authors find humps with high probability of deep eclipses at about 2 day and 0.4 day orbital periods.
\paragraph{}
A sample figure showing eclipse probabilities for FG stars on the main sequence has been reproduced below: