THE MASS-RADIUS RELATION OF YOUNG STARS. I. USCO 5, AN M4.5 ECLIPSING BINARY IN UPPER SCORPIUS OBSERVED BY K2
We present the discovery that UScoCTIO 5, a known spectroscopic binary in the Upper Scorpius star-forming region (P = 34 days, M<inf>tot</inf> sin(i) = 0.64 M⊙), is an eclipsing system with both primary and secondary eclipses apparent in K2 light curves obtained during Campaign 2. We have simultaneously fit the eclipse profiles from the K2 light curves and the existing RV data to demonstrate that UScoCTIO 5 consists of a pair of nearly identical M4.5 stars with M<inf>A</inf> = 0.329 ± 0.002 M⊙,...[Show more]
|Collections||ANU Research Publications|
|Source:||Astrophysical Journal, The|
|01_Kraus_THE_MASS-RADIUS_RELATION_OF_2015.pdf||4.65 MB||Adobe PDF|
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