An unusual very low-mass high-amplitude pre-main sequence periodic variable
M. V. Rodríguez-LedesmaInstitut für Astrophysik, Georg-August-Universität, Friedrich-Hund-Platz 1, 37077 Göttingen, GermanyR. MundtMax-Planck-Institut für Astronomie (MPIA), Königstuhl 17, 69117 Heidelberg, GermanyM. IbrahimovUlugh Bek Astronomical Institute of the Uzbek Academy of Sciences, Astronomicheskaya 33, 700052 Tashkent, UzbekistanS. MessinaINAF – Osservatorio Astrofisico di Catania, via S. Sofia 78, 95123 Catania, ItalyP. PariharIndian Institute of Astrophysics, 560034 Bangalore, IndiaF. V. HessmanInstitut für Astrophysik, Georg-August-Universität, Friedrich-Hund-Platz 1, 37077 Göttingen, GermanyC. Alves de OliveiraHerschel Science Centre, European Space Astronomy Centre (ESA), PO Box 78, 28691 Villanueva de la Cañada, Madrid, SpainW. HerbstAstronomy Department, Wesleyan University, Middletown, CT 06459, USA
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Aims. We have investigated the nature of the variability of CHS 7797, an unusual periodic variable in the Orion Nebula Cluster.
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