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HD 66051, an eclipsing binary hosting a highly peculiar, HgMn-related star
HD 66051 is an eclipsing system with an orbital period of about 4.75 d that exhibits out-of-eclipse variability with the same period. New multicolour photometric observations confirm the longevity of the secondary variations, which we interpret as a signature of surface inhomogeneities on one of the...
| Autores principales: | , , , , , , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
| Publicado: |
Nature Publishing Group UK
2017
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| Materias: | |
| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5517476/ https://www.ncbi.nlm.nih.gov/pubmed/28724922 http://dx.doi.org/10.1038/s41598-017-05987-6 |