E. Yaz Gökçe

MAIN-SEQUENCE EFFECTIVE TEMPERATURES FROM A REVISED MASS–LUMINOSITY RELATION BASED ON ACCURATE PROPERTIES

The mass-luminosity (M-L), mass-radius (M-R) and mass-effective temperature (

The Catalogue of Stellar Parameters from the Detached Double-Lined Eclipsing Binaries in the Milky Way

M-T_{eff}

Solar Space Density of the Red Clump Stars and the Scale-Length of the Thin Disc

) diagrams for a subset of galactic nearby main-sequence stars with masses and radii accurate to

Photometric calibration of the [ α /Fe

\leq 3\%

\alpha\mbox{/Fe}

and luminosities accurate to

] element: I. Calibration with U B V

\leq 30\%

UBV

(268 stars) has led to a putative discovery. Four distinct mass domains have been identified, which we have tentatively associated with low, intermediate, high, and very high mass main-sequence stars, but which nevertheless are clearly separated by three distinct break points at 1.05, 2.4, and 7

photometry

M_{\odot}

Photometric calibration of the [α/Fe] element: I. Calibration with UBV photometry

within the mass range studied of

Local Stellar Kinematics from RAVE data – V. Kinematic Investigation of the Galaxy with Red Clump Stars

0.38-32M_{\odot}