Pierre Maxted p.maxted@keele.ac.uk
Six new compact triply eclipsing triples found with TESS
Maxted, P F L
Authors
Abstract
In this work, we report the discovery and analysis of six new compact triply eclipsing triple star systems found with the TESS mission: TICs 37743815, 42565581, 54060695, 178010808, 242132789, and 456194776. All of these exhibit distinct third-body eclipses where the inner eclipsing binary (EB) occults the third ('tertiary') star, or vice versa. We utilized the TESS photometry, archival photometric data, and available archival spectral energy distribution curves (SED) to solve for the properties of all three stars, as well as many of the orbital elements. We describe in detail our SED fits, search of the archival data for the outer orbital period, and the final global photodynamical analyses. From these analyses, we find that all six systems are coplanar to within 0 degrees-5 degrees, and are viewed nearly edge on (i.e. within a couple of degrees). The outer orbital periods and eccentricities of the six systems are {P-out (days), e}: {68.7, 0.36}, {123, 0.16}, {60.7, 0.01}, {69.0, 0.29}, {41.5, 0.01}, {93.9, 0.29}, respectively, in the order the sources are listed above. The masses of all 12 EB stars were in the range of 0.7-1.8 M-circle dot and were situated near the main sequence. By contrast, the masses and radii of the tertiary stars ranged from 1.5 to 2.3 M-circle dot and 2.9 to 12 R-circle dot, respectively. We use this information to estimate the occurrence rate of compact flat triple systems..
Citation
Maxted, P. F. L., Rappaport, S. A., Borkovits, T., Gagliano, R., Jacobs, T. L., Kostov, V. B., …Stevens, D. J. (2022). Six new compact triply eclipsing triples found with TESS. Monthly Notices of the Royal Astronomical Society, 513(3), 4341-4360. https://doi.org/10.1093/mnras/stac957
Journal Article Type | Article |
---|---|
Acceptance Date | Apr 1, 2022 |
Online Publication Date | Apr 7, 2022 |
Publication Date | 2022-07 |
Publicly Available Date | May 30, 2023 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Publisher | Oxford University Press |
Peer Reviewed | Peer Reviewed |
Volume | 513 |
Issue | 3 |
Pages | 4341-4360 |
DOI | https://doi.org/10.1093/mnras/stac957 |
Keywords | Space and Planetary Science, Astronomy and Astrophysics |
Publisher URL | https://academic.oup.com/mnras/article-abstract/513/3/4341/6564734?redirectedFrom=fulltext |
Files
2204.02539.pdf
(13.6 Mb)
PDF
Publisher Licence URL
https://creativecommons.org/licenses/by-nc/4.0/
stac957.pdf
(3.2 Mb)
PDF
Publisher Licence URL
https://creativecommons.org/licenses/by-nc/4.0/
You might also like
TOI-5678b: A 48-day transiting Neptune-mass planet characterized with CHEOPS and HARPS
(2023)
Journal Article
Refined parameters of the HD 22946 planetary system and the true orbital period of planet d
(2023)
Journal Article
A new dynamical modeling of the WASP-47 system with CHEOPS observations
(2023)
Journal Article
The geometric albedo of the hot Jupiter HD 189733b measured with CHEOPS,
(2023)
Journal Article
Downloadable Citations
About Keele Repository
Administrator e-mail: research.openaccess@keele.ac.uk
This application uses the following open-source libraries:
SheetJS Community Edition
Apache License Version 2.0 (http://www.apache.org/licenses/)
PDF.js
Apache License Version 2.0 (http://www.apache.org/licenses/)
Font Awesome
SIL OFL 1.1 (http://scripts.sil.org/OFL)
MIT License (http://opensource.org/licenses/mit-license.html)
CC BY 3.0 ( http://creativecommons.org/licenses/by/3.0/)
Powered by Worktribe © 2024
Advanced Search