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20072024
most citedInterrelated Main-Sequence Mass-Luminosity, Mass-Radius and Mass-Effective Temperature Relations

265 citations · 567 across the 17 of their papers we have counts for

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Showing astro-ph.SRShow all

10 papers · 1 filter

astro-ph.SR2022★ 5 cited

A Silent Revolution in Fundamental Astrophysics

Z. Eker, F. Soydugan, V. Bakis +2

Arbitrariness in the zero point of bolometric corrections is a nearly century-old paradigm leading to two more paradigms. "Bolometric corrections must always be negative," and "bol…

astro-ph.SR2021★ 13 cited

Standard stellar luminosities; what are typical and limiting accuracies in the era after Gaia?

Z. Eker, F. Soydugan, S. Bilir +1

Methods of obtaining stellar luminosities (L) have been revised and a new concept, standard stellar luminosity, has been defined. Among the three methods (direct method from radii…

astro-ph.SR2021★ 7 cited

On the Zero Point Constant of the Bolometric Correction Scale

Z. Eker, V. Bakis, F. Soydugan +1

Arbitrariness attributed to the zero point constant of the band bolometric corrections () and its relation to "bolometric magnitude of a star ought to be brighter than it…

astro-ph.SR2020★ 3 cited

Kepler Binary Stars in NGC 6819 Open Cluster: KIC 5113146 and KIC 5111815

E. Soydugan, F. Alicavus, F. Soydugan +1

In this study, investigation of two double-lined binary stars KIC 5113146 and KIC 5111815 in NGC 6819 is presented based on both photometric and spectroscopic data. Simultaneous an…

astro-ph.SR2020★ 80 cited

Empirical Bolometric Correction Coefficients for Nearby Main-Sequence Stars in Gaia Era

Z. Eker, F. Soydugan, S. Bilir +6

Nearby detached double-lined eclipsing binaries with most accurate data were studied and 290 systems were found with at least one main-sequence component having a metallicity $0.00…

astro-ph.SR2019★ 7 cited

Investigation of near-contact semi-detached binary W UMi through observations and evolutionary models

Faruk Soydugan, Esin Soydugan, Fahri Aliçavuş

W UMi is a near contact, semi-detached, double-lined eclipsing binary star with an orbital period of 1.7 days. Simultaneous analysis of new BVR multi-color light curves and radial…

astro-ph.SR2018★ 265 cited

Interrelated Main-Sequence Mass-Luminosity, Mass-Radius and Mass-Effective Temperature Relations

Z. Eker, V. Bakis, S. Bilir +7

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-luminosit…

astro-ph.SR2015★ 11 cited

The Galactic Kinematics of Cataclysmic Variables

T. Ak, S. Bilir, A. Özdönmez +5

Kinematical properties of CVs were investigated according to population types and orbital periods, using the space velocities computed from recently updated systemic velocities, pr…

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.SR2009★ 7 cited

The Spectroscopic Orbits of Three Double-lined Eclipsing Binaries: I. BG Ind, IM Mon, RS Sgr

V. Bakis, H. Bakis, S. Bilir +7

We present the spectroscopic orbit solutions of three double-lines eclipsing binaries, BG Ind, IM Mon and RS Sgr. The first precise radial velocities (RVs) of the components were d…