activity
20142024
most citedTesting Multiband (G, GBP, GRP, B, V and TESS) Standard Bolometric Corrections by Recovering Luminosity and Radii of 341 Host Stars

25 citations · 65 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR20242 cited

The Fundamental Parameters and Evolutionary Status of V454 Aurigae

Gökhan Yücel, Remziye Canbay, Volkan Bakış

Eclipsing binary systems have a unique feature, which enables scientists to obtain precise fundamental star parameters, which opens to greater area of astrophysics studies. In this…

astro-ph.SR202325 cited

Testing Multiband (G, GBP, GRP, B, V and TESS) Standard Bolometric Corrections by Recovering Luminosity and Radii of 341 Host Stars

Zeki Eker, Volkan Bakis

Main-sequence bolometric corrections (BC) and a standard BC-Teff relation are produced for TESS wavelengths using published physical parameters and light ratios from SED models of…

astro-ph.HE20236 cited

Discovery of optical emission associated with the supernova remnant G107.5-1.5

Hicran Bakis, Gunay Bulut, Volkan Bakis +2

We present the first results from an imaging and a spectroscopic survey of the optical emission associated with supernova remnant (SNR) G107.51.5. We discovered optical diffuse…

astro-ph.SR20224 cited

Detailed Evolutionary Models for Twins in Sight of New Spectral Data: AN Cam, RS Ari, and V455 Aur

Gökhan Yücel, Volkan Bakış

We present the evolutionary scenarios for three eclipsing twin (1) binary systems using their combined spectroscopic and photometric data. Using accurate \textit{TE…

astro-ph.SR20213 cited

Orbital Period Changes in IO Cep, IM Cep and TX Ari: Path to Masses of Distant Components

V. Bakış, Z. Eker, H. Bakış +7

Three Algol-type binary systems (IO Cep, IM Cep and TX Ari) showing cyclic orbital period changes are studied. The combination of time of minimum data from the ground-based observa…

astro-ph.GA201618 cited

CCD UBV Photometry and Kinematics of the Open Cluster NGC 225

S. Bilir, Z. F. Bostanci, T. Yontan +6

We present the results of CCD photometric and spectroscopic observations of the open cluster NGC 225. In order to determine the structural parameters of NGC 225, we calculate…