activity
20122016
most citedMain-Sequence Effective Temperatures from a Revised Mass-Luminosity Relation Based on Accurate Properties

156 citations · 271 across the 12 of their papers we have counts for

collaborators

13 papers

astro-ph.SR2016★ 3 cited

Photometric Calibration of the [/Fe] Element: I. Calibration with UBV Photometry

S. Karaali, E. Yaz Gokce, S. Bilir

We present the calibration of the [/Fe] element in terms of the ultra-violet excess for 469 dwarf stars with mag corresponding the spectral type range…

astro-ph.SR2015★ 156 cited

Main-Sequence Effective Temperatures from a Revised Mass-Luminosity Relation Based on Accurate Properties

Z. Eker, F. Soydugan, E. Soydugan +6

The mass-luminosity (M-L), mass-radius (M-R) and mass-effective temperature () diagrams for a subset of galactic nearby main-sequence stars with masses and radii accurat…

astro-ph.SR2014

Effective Temperatures of Selected Main-sequence Stars with Most Accurate Parameters

F. Soydugan, Z. Eker, E. Soydugan +6

In this study, the distributions of the double-lined detached binaries (DBs) on the planes of mass-luminosity, mass radius and mass-effective temperature have been studied. We impr…

astro-ph.GA2014

Absolute Magnitude Calibration for Dwarfs Based on the Colour-Magnitude Diagrams of Galactic Clusters

S. Karaali, E. Yaz Gokce, S. Bilir +1

We present two absolute magnitude calibrations for dwarfs based on colour-magnitude diagrams of Galactic clusters. The combination of the absolute magnitudes of the dwarf fid…

astro-ph.SR2014★ 72 cited

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

Z. Eker, S. Bilir, F. Soydugan +5

The most accurate stellar astrophysical parameters were collected from the solutions of the light and the radial velocity curves of 257 detached double-lined eclipsing binaries in…

astro-ph.GA2014★ 3 cited

Colour Transformations between BVRc and g'r'i' Photometric Systems for Giant Stars

S. Ak, T. Ak, S. Karaali +9

The transformation equations from to magnitudes and vice versa for the giants were established from a sample of 80 stars collected from Soubiran et al. (2010) with…