Accurate stellar parameters for stars in Tight Triple Systems
| Autor: | Moharana, Ayush, Hełminiak, K.G., Marcadon, F., Pawar, T., Konacki, M. |
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| Rok vydání: | 2021 |
| Předmět: | |
| ISSN: | 1538-4365 |
| DOI: | 10.5281/zenodo.5123520 |
| Popis: | Tight Triple Systems (TTS) have stars in a hierarchical configuration with a third star orbiting the inner binary with a period of fewer than 1000 days. Such systems are a hub of various dynamical interactions and are important for understanding the formation and evolution of stars in multiple systems. Having a detached eclipsing binary (DEB) as one of its components allows us to obtain precise stellar and orbital parameters of these systems. Various recent discoveries have been due to space-based photometry from Kepler and TESS. We present the accurate stellar and orbital parameters of a TTS, TIC 284595199, using TESS photometry coupled with radial velocities extracted from the triple-lined (SB3) spectra from HIDES spectrograph. Using these accurate parameters we determine the evolutionary states of the stars and the dynamic interactions possible in this system. {"references":["Hajdu et al., 2017, MNRAS, 471, 1230 (https://doi.org/10.1093/mnras/stx1523)","Izumiura et al., 1999, in Proc. EAMA, 77","Conroy et al., 2020, ApJS, 250, 34 (https://doi.org/10.3847/1538-4365/abb4e2)","Mazeh & Zucker, 1994, Ap&SS, 212, 349 (https://doi,org/10.1007/BF00984538 )","Konacki et al., 2009, ApJ, 704, 513 (https://doi.org/10.1088/0004-637X/704/1/513)","Choi et al., 2016, ApJ, 823,102 (https://doi.org/10.3847/0004-637X/823/2/102)","Toonen et al., 2020, A&A, 640, A16 (https://doi.org/10.1051/0004-6361/201936835)"]} |
| Databáze: | OpenAIRE |
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