A KELT–TESS Eclipsing Binary in a Young Triple System Associated with the Local “Stellar String” Theia 301

• Published in: The Astronomical journal 2020-10, Vol.160 (4), p.187
• Main Authors: Cunningham, Joni-Marie C., Feliz, Dax L., Dixon, Don M., Pepper, Joshua, Stassun, Keivan G., Siverd, Robert J., Zhou, George, Bayliss, Daniel, Tan, Thiam-Guan, Cargile, Phillip, James, David, Kuhn, Rudolf B., Kounkel, Marina
• Format: Article
• Language: English
• Subjects: ABSORPTION; Age; Astronomy; ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; BENCHMARKS; Companion stars; ECLIPSE; Eclipsing binary stars; EMISSION; Fundamental parameters of stars; LITHIUM; Low mass stars; LUMINOSITY; MASS; ORBITS; PROPER MOTION; STAR EVOLUTION; STARS; Stellar age; Stellar associations; Strings; X RADIATION; X-ray emissions
• ISSN: 0004-6256; 1538-3881; 1538-3881
• DOI: 10.3847/1538-3881/abafaf

HD 54236 is a nearby, wide common-proper-motion visual pair that has been previously identified as likely being very young by virtue of strong X-ray emission and lithium absorption. Here, we report the discovery that the brighter member of the wide pair, HD 54236A, is itself an eclipsing binary (EB), comprising two near-equal solar-mass stars on a 2.4 days orbit. It represents a potentially valuable opportunity to expand the number of benchmark-grade EBs at young stellar ages. Using new observations of Ca ii  H and K emission and lithium absorption in the wide K-dwarf companion, HD 54236B, we obtain a robust age estimate of 225 ± 50 Myr for the system. This age estimate and Gaia proper motions show HD 54236 is associated with Theia 301, a newly discovered local “stellar string,” which itself may be related to the AB Dor moving group through shared stellar members. Applying this age estimate to AB Dor itself alleviates reported tension between observation and theory that arises for the luminosity of AB Dor C when younger age estimates are used.