Orbital and Stellar Parameters for 2M06464003+0109157: A Double-lined Eclipsing Binary of Spotted, Sub-solar Twins

We calculated physical and orbital properties for 2M06464003+0109157, a 1.06 day eclipsing double lined spectroscopic binary. We modeled the system's ASAS-SN and TESS light curves, measuring the system's inclination and radii of each component. Extracting radial velocities for each component from 6 SDSS/APOGEE spectra, we measured the system's mass ratio and performed a full orbital fit. Our analysis indicates that 2M06464003+0109157 has components with nearly equal masses (m(1)/m(2) = 0.99 0.01; M-1,M-2 = 0.57 0.015 M-circle dot) and comparable radii (R-1 = 0.66 0.05 R-circle dot, R-2 = 0.57 0.06 R-circle dot). The solution required two star spots to incorporate the out of eclipse variation that is seen in the light curve. We report our full characterization of this system, and prospects for similar analyses using survey data to measure precise physical and orbital properties for EBs.

Automated summary

This study calculated and modeled the physical and orbital properties of 2M06464003+0109157, a double lined spectroscopic binary. The analysis showed components with nearly equal masses and comparable radii, requiring the inclusion of star spots to explain eclipse variations in the light curve. The research highlights the potential for similar analyses using survey data to measure precise properties for eclipsing binaries.