For low -
mass eclipsing binary stars, the method of eclipse minimum timing allows astronomers to search for smaller masses than those feasible with radial velocity measurements.
Not exact matches
Among the undiluted
binaries, planet - like
eclipses may be caused by grazing EBs and the (central)
eclipses of two stellar components with large ratios in area or surface brightness, typically due to a large
mass ratio.
Specifically,
eclipsing binary stars can be used to study the stellar
mass - radius relationship and to test predictions of theoretical stellar evolution models.
We measure
eclipse timing variations (ETVs), which are then combined with the single - lined radial velocity measurements to yield
masses in a manner equivalent to double - lined spectroscopic
binaries.