Eker, ZekiBakis, VolkanBilir, SelcukSoydugan, FarukSteer, IanSoydugan, EsinBakis, Hicran2025-01-272025-01-272018978-0-7354-1768-70094-243Xhttps://doi.org/10.1063/1.5078888https://hdl.handle.net/20.500.12428/2070734th International Physics Congress (IPS) of the Turkish-Physical-Society (TPS) -- SEP 05-09, 2018 -- Konacik, TURKEYConventional mass- luminosity (M- L) relations are defined using 509 nearby main- sequence (MS) stars within the Solar neighborhood. A smooth mass- radius (M- R) relation was fixed from radii of MS stars appeared in literature having masses within the limits 0.179- 1.5 M. Similarly, a smooth mass- effective temperature (M- Teff) relation was derived for the main- sequence stars having masses within the limits 1.5- 31 M using their effective temperatures available. The omitted parts of M- R and M- Teff relations in the range from 0.179 to 31 M were computed according to Stephan- Boltzmann law, so inter- related M- L, M- R and M- Teff were achieved.eninfo:eu-repo/semantics/closedAccesscataloguesbinaries: eclipsingbinaries: spectroscopicbinaries: detachedstars: fundamental parametersConference Object204210.1063/1.5078888N/AWOS:0004683589000162-s2.0-85057161853Q4