The mass of a star is the most fundamental parameter for its structure, evolution, and final
fate. It is particularly important for any kind of stellar archaeology and characterization of …

Absolute parameters of 509 main-sequence stars selected from the components of detached
eclipsing spectroscopic binaries in the solar neighbourhood are used to study mass …

The mass-luminosity (ML), mass-radius (MR) and mass-effective temperature ($ M-T_ {eff} $)
diagrams for a subset of galactic nearby main-sequence stars with masses and radii …

In this work, we have taken advantage of the most recent accurate stellar characterizations
carried out using asteroseismology, eclipsing binaries and interferometry to evaluate a …

Methods of obtaining stellar luminosities (L) have been revised and a new concept, standard
stellar luminosity, has been defined. In this paper, we study three methods:(i) a direct …

Developments on various relations among stellar variables such as the main sequence
empirical mass-luminosity (MLR), massradius (MRR) and mass-effective temperature (MTR) …

Context. Scaling relations are very useful tools for estimating unknown stellar quantities.
Within this framework, eclipsing binaries are ideal for this goal because their mass and …

Context. Estimating stellar masses and radii for most stars is a challenge, but it is critical to
know them for many different astrophysical fields, such as exoplanet characterization or …

Stellar evolutionary models simulate well binary stars when individual stellar mass and
system metallicity are known. The mass can be derived directly from observations only in the …

In this study, we have investigated the stellar parameters of Algol‐type eclipsing binaries in
the range of primary and secondary masses between 0.2 and 8 M⊙, which were obtained …