A study of nine compact triply eclipsing triples. Issue 1 (2nd February 2023)

• Record Type: Journal Article
• Authors: Rappaport, S A; Borkovits, T; Gagliano, R; Jacobs, T L; Tokovinin, A; Mitnyan, T; Komžík, R; Kostov, V B; Powell, B P; Torres, G; Terentev, I; Omohundro, M; Pribulla, T; Vanderburg, A; Kristiansen, M H; Latham, D; Schwengeler, H M; LaCourse, D; Bíró, I B; Csányi, I; Czavalinga, D R; Garai, Z; Pál, A; Rodriguez, J E; Stevens, D J
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 521:Issue 1(2023)
• Page Start: 558
• Page End: 584
• Publication Date: 2023-02-02
• Subjects: binaries (including multiple): close -- binaries: eclipsing -- stars: individual: TIC 47151245 -- stars: individual: TIC 81525800 -- stars: individual: TIC 99013269 -- stars: individual: TIC 229785001; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stad367
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: In this work, we report the independent discovery and analysis of nine new compact triply eclipsing triple star systems found with the Transiting Exoplanet Survey Satellite ( TESS ) mission: TICs 47151245, 81525800, 99013269, 229785001, 276162169, 280883908, 294803663, 332521671, and 356324779. Each of these nine systems exhibits distinct third-body eclipses where the third ('tertiary') star occults the inner eclipsing binary (EB), or vice versa. We utilize a photodynamical analysis of the TESS photometry, archival photometric data, TESS eclipse timing variations of the EBs, available archival spectral energy distribution (SED) curves, and, in some cases, newly acquired radial velocity observations, to solve for the parameters of all three stars, as well as most of the orbital elements. From these analyses we find that the outer orbits of all nine systems are viewed nearly edge on (i.e. within ≲4°), and six of the systems are coplanar to within 5°; the others have mutual inclination angles of 20°, 41°, and possibly 179° (i.e. a retrograde outer orbit). The outer orbital periods range from 47.8 to 604 d, with eccentricities spanning 0.004–0.61. The masses of all 18 EB stars are in the range of 0.9–2.6 M⊙ and are mostly situated near the main sequence. By contrast, the masses and radii of the tertiary stars range from 1.4 to 2.8 M⊙ and 1.5 to 13 R⊙, respectively. We make use of the system parameters from these nine systems, plus those from a comparable number of compact triply eclipsing triples published previously, to gain some statistical insight into their properties.