An extreme-mass ratio, short-period eclipsing binary consisting of a B dwarf primary and a pre-main-sequence M star companion discovered by KELT

Daniel J. Stevens(Pennsylvania State University), Keivan G. Stassun(Vanderbilt University), David W. Latham(Center for Astrophysics Harvard & Smithsonian), Michael B. Lund, Mark Manner(Spot Observatory), Karen A. Collins(Center for Astrophysics Harvard & Smithsonian), M. Calkins(Center for Astrophysics Harvard & Smithsonian), Thomas G. Beatty(University of Arizona), Rudolf B. Kuhn, Gilbert A. Esquerdo(Center for Astrophysics Harvard & Smithsonian), Marshall C. Johnson(The Ohio State University), Jason T. Wright(Pennsylvania State University), Robert J. Siverd(Gemini North Observatory), George Zhou(University of Southern Queensland), Patcharapol Wachiraphan(University of Colorado Boulder), Steven Villanueva(Goddard Space Flight Center), John F. Kielkopf(University of Louisville), Adam L. Kraus(Center for Astrophysics Harvard & Smithsonian), B. Scott Gaudi(The Ohio State University), Aaron C. Rizzuto(Dairy Australia (Australia)), Allyson Bieryla(Center for Astrophysics Harvard & Smithsonian), Joshua Pepper(Lehigh University)

Monthly Notices of the Royal Astronomical Society

October 10, 2020

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