TY  - GEN 
AU  - Claret, A.
PY  - 2023
UR  - https://hdl.handle.net/10481/83238
AB  - Aims. One of the most reliable means of studying the stellar interior is through the apsidal motion in double line eclipsing binary systems since these systems present errors in masses, radii, and effective temperatures of only a few per cent. On the...
LA  - eng
PB  - EDP Sciences
KW  - Binaries: close
KW  - Binaries: eclipsing
KW  - Stars: evolution
KW  - Stars: interiors
TI  - Theoretical tidal evolution constants for stellar models from the pre-main sequence to the white dwarf stage: Apsidal motion constants, moment of inertia, and gravitational potential energy
DO  - 10.1051/0004-6361/202346250
ER  -