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The characterisation of detached eclipsing binaries with low mass components has become important when verifying the role of convection in stellar evolutionary models, which requires model-independent measurements of stellar parameters with great pre
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::45b60f1500891927e312535082645bf0
http://arxiv.org/abs/2206.08708
http://arxiv.org/abs/2206.08708
Publikováno v:
Research Notes of the AAS. 6:172
Eclipsing binaries allow the study of physical stellar parameters in a model-independent way, when photometric and spectroscopic data are combined. However, when spectroscopic data are not available, purely photometric methods can be adopted to first