作者: L. Tal-Or , M. Fridlund , M. Fridlund , B. Tingley , B. Tingley
DOI: 10.1051/0004-6361/201220862
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摘要: We present the study of CoRoT transiting planet candidate 101186644, also named LRc01_E1\₄780. Analysis lightcurve and HARPS spectroscopic follow-up observations this faint (m(V) = 16) revealed an eclipsing binary composed a late F-type primary (T-eff 6090 +/- 200 K) low-mass, dense M-dwarf secondary on eccentric (e 0.4) orbit with period similar to 20.7 days. The has mass 0.096 0.011 M-circle dot, radius 0.104(-0.006)(+0.026) R-circle which possibly makes it smallest densest reported so far. Unlike claim that theoretical models predict radii are 5-15% smaller than measured for low-mass stars, one seems have is consistent might even be below predicted by models.