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Updated: Dec 22, 2025

Setting Limits on Supersymmetry Using Simplified Models
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Comentario sobre "Un sistema binario de estrellas gigantes y agujeros negros de baja masa que no interactúa"

Ed P J van den Heuvel1, Thomas M Tauris2,3

  • 1Anton Pannekoek Institute for Astronomy, University of Amsterdam, 1098 XH Amsterdam, Netherlands. e.p.j.vandenheuvel@uva.nl.

Science (New York, N.Y.)
|May 9, 2020
PubMed
Resumen

Proponemos que el compañero invisible de la estrella gigante roja 2MASS J05215658+4359220 puede ser un sistema estelar binario, no un agujero negro. Esta hipótesis de estrella binaria explica la falta de emisiones de rayos X detectadas desde el sistema.

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