Detailed Evolutionary Models for Twins in Sight of New Spectral Data: AN Cam, RS Ari, and V455 Aur
G\"okhan Y\"ucel, Volkan Bak{\i}\c{s}

TL;DR
This study models the detailed evolutionary history of three twin binary star systems using combined spectroscopic and photometric data, providing precise parameters and evolutionary stages for each system.
Contribution
It presents the first detailed evolutionary scenarios for these systems using high-precision data and the MESA code, highlighting their current states and future evolution.
Findings
AN Cam components have passed the terminal age main-sequence.
RS Ari's primary is in the giant phase, secondary has passed the main-sequence.
V455 Aur's components are still on the main-sequence.
Abstract
We present the evolutionary scenarios for three eclipsing twin (1) binary systems using their combined spectroscopic and photometric data. Using accurate \textit{TESS} photometric data, RV measurements, and spectroscopic data enabled us to calculate fundamental parameters, such as mass and radius, better than 2 percent. The temperature of each component and metallicity of the systems have been obtained via high-resolution spectra. According to our spectral analysis, the metallicity values of AN Cam, RS Ari, and V455 Aur are \text{[M/H]}=\,0.000.12, 0.050.08, and -0.070.07, respectively. Using the derived metallicity for each system, initial orbital parameters and detailed evolutionary status of these three systems are calculated with high precision by using \textsc{mesa}. According to our analysis, both components of AN Cam have passed the terminal age…
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Taxonomy
TopicsAstronomical and nuclear sciences
