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Four new self-lensing binaries from Kepler: Radial velocity characterization and astrophysical implications

Published online by Cambridge University Press:  09 October 2020

Kento Masuda Open the ORCID record for Kento Masuda [Opens in a new window] ,
Hajime Kawahara ,
David W. Latham ,
Allyson Bieryla ,
Morgan MacLeod ,
Masanobu Kunitomo ,
Othman Benomar  and
Wako Aoki
Kento Masuda
Affiliation:
Institute for Advanced Study, Princeton, NJ08540, USA email: kmasuda@ias.edu
Hajime Kawahara
Affiliation:
Department of Earth and Planetary Science, The University of Tokyo, Tokyo113-0033, Japan Research Center for the Early Universe, School of Science, The University of Tokyo, Tokyo113-0033, Japan email: kawahara@eps.s.u-tokyo.ac.jp
David W. Latham
Affiliation:
Center for Astrophysics | Harvard & Smithsonian, Cambridge, MA02138, USA
Allyson Bieryla
Affiliation:
Center for Astrophysics | Harvard & Smithsonian, Cambridge, MA02138, USA
Morgan MacLeod
Affiliation:
Center for Astrophysics | Harvard & Smithsonian, Cambridge, MA02138, USA
Masanobu Kunitomo
Affiliation:
Department of Physics, School of Medicine, Kurume University, Fukuoka830-0011, Japan
Othman Benomar
Affiliation:
National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo181-8588, Japan
Wako Aoki
Affiliation:
National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo181-8588, Japan
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In Kawahara et al. (2018) and Masuda et al. (2019), we reported the discovery of four self-lensing binaries consisting of F/G-type stars and (most likely) white dwarfs whose masses range from 0.2 to 0.6 solar masses. Here we present their updated system parameters based on new radial velocity data from the Tillinghast Reflector Echelle Spectrograph at the Fred Lawrence Whipple Observatory, and the Gaia parallaxes and spectroscopic parameters of the primary stars. We also briefly discuss the astrophysical implications of these findings.

Keywords

binaries: eclipsingblue stragglersgravitational lensingtechniques: radial velocitieswhite dwarfs
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S357: White Dwarfs as Probes of Fundamental Physics: Tracers of Planetary, Stellar and Galactic Evolution , October 2019 , pp. 215 - 219
Copyright
© International Astronomical Union 2020

References

Cui, X.-Q., Zhao, Y.-H., Chu, Y.-Q., et al. 2012, RAA, 12, 1197Google Scholar
Kawahara, H. & Masuda, K. 2019, AJ, 157, 218CrossRefGoogle Scholar
Kawahara, H., Masuda, K., MacLeod, M., et al. 2018, AJ, 155, 144CrossRefGoogle Scholar
Kruse, E. & Agol, E. 2014, Science, 344, 275CrossRefGoogle Scholar
Lin, J., Rappaport, S., Podsiadlowski, P., et al. 2011, ApJ, 732, 70CrossRefGoogle Scholar
Luo, A.-L., Zhao, Y.-H., Zhao, G., et al. 2015, RAA, 15, 1095Google Scholar
Marsh, T. R., Dhillon, V. S., & Duck, S. R. 1995, MNRAS, 275, 828CrossRefGoogle Scholar
Masuda, K., Kawahara, H., Latham, D. W., et al. 2019, ApJ (Letters), 881, L3Google Scholar
Mink, D. J. 2011, in Astronomical Society of the Pacific Conference Series, Vol. 442, Astronomical Data Analysis Software and Systems XX, ed. I. N. Evans, A. Accomazzi, D. J. Mink, & A. H. Rots, 305Google Scholar
Noguchi, K., Aoki, W., Kawanomoto, S., et al. 2002, PASJ, 54, 855CrossRefGoogle Scholar
Szentgyorgyi, A. H. & Furész, G. 2007, in Revista Mexicana de Astronomia y Astrofisica, vol. 27, Vol. 28, Revista Mexicana de Astronomia y Astrofisica Conference Series, ed. S. Kurtz, 129–133Google Scholar
Trimble, V. L. & Thorne, K. S. 1969, ApJ, 156, 1013CrossRefGoogle Scholar
Vos, J., Zorotovic, M., Vučković, M., Schreiber, M. R., & Østensen, R. 2018, MNRAS, 477, L40CrossRefGoogle Scholar
Yahalomi, D. A., Shvartzvald, Y., Agol, E., et al. 2019, ApJ, 880, 33CrossRefGoogle Scholar
Yee, S. W., Petigura, E. A., & von Braun, K. 2017, ApJ, 836, 77CrossRefGoogle Scholar