Program: GS-2020A-Q-140
| Title: | Eclipsing Binaries from TESS |
| PI: | Eunkyu Han |
| Co-I(s): | Gregory Mace |
Abstract
Double-lined (SB2) eclipsing binaries (EBs) offer the best way to empirically determine mass-radius relationship for M dwarfs. However, empirical measurements from SB2 EBs often show larger than expected radii for their measured mass, metallicity and age.