A dense 0.1-solar-mass star in a 51-minute-orbital-period eclipsing binary - Nature

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A dense 0.1-solar-mass star in a 51-minute-orbital-period eclipsing binary - Nature
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Nature research paper: A dense 0.1-solar-mass star in a 51-minute-orbital-period eclipsing binary

K.B.B. is a Pappalardo Postdoctoral Fellow in Physics at MIT and thanks the Pappalardo fellowship programme for supporting his research. The design and construction of HiPERCAM was funded by the European Research Council under the European Union’s Seventh Framework Programme under ERC-2013-ADG grant agreement number 340040 . V.S.D. and HiPERCAM operations are supported by STFC grant ST/V000853/1. T.R.M. and B.T.G.

Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USACenter for Astrophysics, Harvard & Smithsonian, Cambridge, MA, USAMax-Planck Institute for Astronomy, Heidelberg, GermanyThomas R. Marsh & Boris T. Gänsicke Division of Physics, Mathematics and Astronomy, California Institute of Technology, Pasadena, CA, USA

Ilaria Caiazzo, Jim Fuller, Matthew J. Graham, S. R. Kulkarni, Jan van Roestel, Andrew J. Drake & Thomas A. PrinceV. S. Dhillon & S. P. LittlefairAstronomical Observatory, University of Warsaw, Warszawa, PolandPablo Rodríguez-GilCaltech Optical Observatories, California Institute of Technology, Pasadena, CA, USAIPAC, California Institute of Technology, Pasadena, CA, USA

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