EPIC 219217635

A doubly eclipsing quadruple system containing an evolved binary

T. Borkovits, S. Albrecht, S. Rappaport, L. Nelson, A. Vanderburg, B. L. Gary, T. G. Tan, A. B. Justesen, M. H. Kristiansen, T. L. Jacobs, D. LaCourse, H. Ngo, N. Wallack, G. Ruane, D. Mawet, S. B. Howell, R. Tronsgaard

Research output: Contribution to journalArticle

3 Citations (Scopus)

Abstract

We have discovered a doubly eclipsing, bound, quadruple star system in the field of K2 Campaign 7. EPIC 219217635 is a stellar image with Kp = 12.7 that contains an eclipsing binary (EB) with PA = 3.59470 d and a second EB with PB = 0.61825 d. We have obtained follow-up radial velocity (RV) spectroscopy observations, adaptive optics imaging, and ground-based photometric observations. From our analysis of all the observations, we derive good estimates for a number of the system parameters. We conclude that (1) both binaries are bound in a quadruple star system; (2) a linear trend to the RV curve of binary A is found over a 2-yr interval, corresponding to an acceleration, γ˙ = 0.0024 ± 0.0007 cm s-2; (3) small irregular variations are seen in the eclipse timing variations (ETVs) detected over the same interval; (4) the orbital separation of the quadruple system is probably in the range of 8-25 au; and (5) the orbital planes of the two binaries must be inclined with respect to each other by at least 25°. In addition, we find that binary B is evolved, and the cooler and currently less massive star has transferred much of its envelope to the currently more massive star. We have also demonstrated that the system is sufficiently bright that the eclipses can be followed using small ground-based telescopes, and that this system may be profitably studied over the next decade when the outer orbit of the quadruple is expected to manifest itself in the ETV and/or RV curves.

Original languageEnglish
Pages (from-to)5135-5152
Number of pages18
JournalMonthly Notices of the Royal Astronomical Society
Volume478
Issue number4
DOIs
Publication statusPublished - Aug 21 2018

Fingerprint

eclipses
radial velocity
massive stars
time measurement
intervals
stars
orbitals
curves
coolers
adaptive optics
envelopes
spectroscopy
telescopes
orbits
trends
estimates

Keywords

  • Binaries: close
  • Binaries: eclipsing
  • Binaries: general

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Borkovits, T., Albrecht, S., Rappaport, S., Nelson, L., Vanderburg, A., Gary, B. L., ... Tronsgaard, R. (2018). EPIC 219217635: A doubly eclipsing quadruple system containing an evolved binary. Monthly Notices of the Royal Astronomical Society, 478(4), 5135-5152. https://doi.org/10.1093/mnras/sty1386

EPIC 219217635 : A doubly eclipsing quadruple system containing an evolved binary. / Borkovits, T.; Albrecht, S.; Rappaport, S.; Nelson, L.; Vanderburg, A.; Gary, B. L.; Tan, T. G.; Justesen, A. B.; Kristiansen, M. H.; Jacobs, T. L.; LaCourse, D.; Ngo, H.; Wallack, N.; Ruane, G.; Mawet, D.; Howell, S. B.; Tronsgaard, R.

In: Monthly Notices of the Royal Astronomical Society, Vol. 478, No. 4, 21.08.2018, p. 5135-5152.

Research output: Contribution to journalArticle

Borkovits, T, Albrecht, S, Rappaport, S, Nelson, L, Vanderburg, A, Gary, BL, Tan, TG, Justesen, AB, Kristiansen, MH, Jacobs, TL, LaCourse, D, Ngo, H, Wallack, N, Ruane, G, Mawet, D, Howell, SB & Tronsgaard, R 2018, 'EPIC 219217635: A doubly eclipsing quadruple system containing an evolved binary', Monthly Notices of the Royal Astronomical Society, vol. 478, no. 4, pp. 5135-5152. https://doi.org/10.1093/mnras/sty1386
Borkovits, T. ; Albrecht, S. ; Rappaport, S. ; Nelson, L. ; Vanderburg, A. ; Gary, B. L. ; Tan, T. G. ; Justesen, A. B. ; Kristiansen, M. H. ; Jacobs, T. L. ; LaCourse, D. ; Ngo, H. ; Wallack, N. ; Ruane, G. ; Mawet, D. ; Howell, S. B. ; Tronsgaard, R. / EPIC 219217635 : A doubly eclipsing quadruple system containing an evolved binary. In: Monthly Notices of the Royal Astronomical Society. 2018 ; Vol. 478, No. 4. pp. 5135-5152.
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AU - Albrecht, S.

AU - Rappaport, S.

AU - Nelson, L.

AU - Vanderburg, A.

AU - Gary, B. L.

AU - Tan, T. G.

AU - Justesen, A. B.

AU - Kristiansen, M. H.

AU - Jacobs, T. L.

AU - LaCourse, D.

AU - Ngo, H.

AU - Wallack, N.

AU - Ruane, G.

AU - Mawet, D.

AU - Howell, S. B.

AU - Tronsgaard, R.

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N2 - We have discovered a doubly eclipsing, bound, quadruple star system in the field of K2 Campaign 7. EPIC 219217635 is a stellar image with Kp = 12.7 that contains an eclipsing binary (EB) with PA = 3.59470 d and a second EB with PB = 0.61825 d. We have obtained follow-up radial velocity (RV) spectroscopy observations, adaptive optics imaging, and ground-based photometric observations. From our analysis of all the observations, we derive good estimates for a number of the system parameters. We conclude that (1) both binaries are bound in a quadruple star system; (2) a linear trend to the RV curve of binary A is found over a 2-yr interval, corresponding to an acceleration, γ˙ = 0.0024 ± 0.0007 cm s-2; (3) small irregular variations are seen in the eclipse timing variations (ETVs) detected over the same interval; (4) the orbital separation of the quadruple system is probably in the range of 8-25 au; and (5) the orbital planes of the two binaries must be inclined with respect to each other by at least 25°. In addition, we find that binary B is evolved, and the cooler and currently less massive star has transferred much of its envelope to the currently more massive star. We have also demonstrated that the system is sufficiently bright that the eclipses can be followed using small ground-based telescopes, and that this system may be profitably studied over the next decade when the outer orbit of the quadruple is expected to manifest itself in the ETV and/or RV curves.

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KW - Binaries: close

KW - Binaries: eclipsing

KW - Binaries: general

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