Abstract
This study describes the nature of HD 345723, a variable star identified in TESS photometric data. Analyzing the light curve, we obtain a period of 19 hr and 17 minutes in phase domain. The star, a K6 spectral class, suggest that the variation is due to the presence of large stellar spots in a very close binary system, detected by GAIA spectrum. The double star, at coordinates R.A. (J2000) 20:06:51.33 and decl. (J2000) +22:39:51.7, has a distance of 719 pc, according to reliable GAIA parallax measurements.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
