Detection Of Giant Planets Around Eclipsing Binary Systems
Deviations from strict periodicity of eclipsing binary minimum times have long been known to be caused by the presence of additional bodies near the system. Giant plan- ets orbiting around both binary components would add a beat frequency to observed minimum times, given by their orbital period. For low-mass eclipsing binary systems, such timing
Deeg, H. J. et al.
Fecha de publicación:
0
2002