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A Dearth of Stellar Companions to M-dwarf TESS Objects of Interest
- Publication Year :
- 2021
- Publisher :
- Zenodo, 2021.
-
Abstract
- The Transiting Exoplanet Survey Satellite (TESS) has proven to be a powerful resource for uncovering planets, and the M-dwarfs have been established as favorable planet hosts. It has also become apparent that stellar multiplicity has wide-ranging implications for exoplanet detection and characterization, and that speckle imaging is one of the most efficient tools for probing these multi-star systems. We therefore present high-resolution imaging observations of 63 M-dwarf TOIs using speckle imagers at the 3.5m WIYN telescope, the 4.3m Lowell Discovery Telescope (LDT), and the twin 8.1m Gemini North and South telescopes. However, only one companion was detected. This finding is in contrast to the established 46% binarity rate in exoplanet host stars and the established 27% stellar multiplicity rate for field M-dwarfs. These results indicate that M-dwarf TOIs have a much lower multiplicity rate than field M-dwarfs. Our observations also imply that planet signals detected from M-dwarf TOIs are more likely to be real than those from higher-mass stars. Finally, these data support the observation that exoplanet-hosting binary stars have, in general, wider separations than field binaries.<br />{"references":["Bouma, L. G., Masuda, K., & Winn, J. N. 2018, AJ, 155, 244","Ciardi, D. R., Beichman, C. A., Horch, E. P., & Howell, S. B. 2015, ApJ, 805, 16","Clark, C. A., van Belle, G. T., Horch, E. P., et al. 2020, in Society of Photo-Optical Instrumentation Engineers(SPIE) Conference Series, Vol. 11446, Society ofPhoto-Optical Instrumentation Engineers (SPIE) Conference Series, 114462A","Deacon, N. R., Kraus, A. L., Mann, A. W., et al. 2016, MNRAS, 455, 4212","Furlan, E., & Howell, S. B. 2020, ApJ, 898, 47","Horch, E. P., Veillette, D. R., Baena Gallé, R., et al. 2009, AJ, 137, 5057","Horch, E. P., Howell, S. B., Everett, M. E., & Ciardi, D. R. 2014, ApJ, 795, 60","Howell, S. B., Everett, M. E., Sherry, W., Horch, E., & Ciardi, D. R. 2011, AJ, 142, 19","Howell, S. B. 2020, Frontiers in Astronomy and Space Sciences, 7, 10","Howell, S. B., Matson, R. A., Ciardi, D. R., et al. 2021, AJ, 161, 164","Lund, M. B., & Ciardi, D. 2020, in American Astronomical Society Meeting Abstracts, Vol. 235, American Astronomical Society Meeting Abstracts #235, 249.06","Matson, R. A., Howell, S. B., Horch, E. P., & Everett, M. E. 2018, AJ, 156, 31","Ricker, G. R., Winn, J. N., Vanderspek, R., et al. 2015, Journal of Astronomical Telescopes, Instruments, and Systems, 1, 014003","Teske, J. K., Ciardi, D. R., Howell, S. B., Hirsch, L. A., & Johnson, R. A. 2018, AJ, 156, 292","Winters, J. G., Henry, T. J., Jao, W.-C., et al. 2019, AJ, 157, 216","Ziegler, C., Law, N. M., Baranec, C., et al. 2018, AJ, 156, 259"]}
- Subjects :
- Stellar Astrophysics
Exoplanets
Binaries
Astrophysics::Instrumentation and Methods for Astrophysics
Astrophysics::Solar and Stellar Astrophysics
Astrophysics::Cosmology and Extragalactic Astrophysics
Astrophysics::Earth and Planetary Astrophysics
Low-Mass Stars
High Angular Resolution
Astrophysics::Galaxy Astrophysics
Subjects
Details
- Database :
- OpenAIRE
- Accession number :
- edsair.doi.dedup.....81122facf2fe2f27e399b0ee806207de
- Full Text :
- https://doi.org/10.5281/zenodo.5129301