Image Details
Caption: Figure 11.
SED fitting of total eclipsing binary with model of KURUCZ and the obtained Teff is 6500 K. The best-fit model is overplotted on the observed flux points across UV to IR wavelengths. The elevated χ2 value likely arises from the infrared excess observed in the WISE bands, hinting at potential circumstellar material or a third body.
© 2026. The Author(s). Published by the American Astronomical Society.