A 2+1+1 quadruple star system containing the most eccentric, low-mass, short-period, eclipsing binary known

E. Han*, S. A. Rappaport, A. Vanderburg, B. M. Tofflemire, T. Borkovits, H. M. Schwengeler, P Zasche, D. M. Krolikowski, P. S. Muirhead, M. H. Kristiansen, I. A. Terentev, M. Omohundro, R Gagliano, T Jacobs, D LaCourse

*Corresponding author for this work

Research output: Contribution to journalJournal articleResearchpeer-review

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Original languageEnglish
JournalMonthly Notices of the Royal Astronomical Society
ISSN0035-8711
DOIs
Publication statusAccepted/In press - 2022

Keywords

  • Stars: binaries: close
  • Stars: binaries: eclipsing
  • Stars: binaries: general
  • Stars: late-type
  • Stars: low-mass

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