NGTS-EB-7, an eccentric, long-period, low-mass eclipsing binary
(2024)
Journal Article
Rodel, T., Watson, C. A., Ulmer-Moll, S., Gill, S., Maxted, P. F. L., Casewell, S. L., Brahm, R., Wilson, T. G., Costes, J. C., Eschen, Y. N. E., Doyle, L., Freckelton, A. V., Alves, D. R., Apergis, I., Bayliss, D., Bouchy, F., Burleigh, M. R., Dumusque, X., Eberhardt, J., Fernández, J. F., …Wheatley, P. J. (in press). NGTS-EB-7, an eccentric, long-period, low-mass eclipsing binary. Monthly Notices of the Royal Astronomical Society, 1-22. https://doi.org/10.1093/mnras/stae2799
Despite being the most common types of stars in the Galaxy, the physical properties of late M dwarfs are often poorly constrained. A trend of radius inflation compared to evolutionary models has been observed for earlier type M dwarfs in eclipsing bi... Read More about NGTS-EB-7, an eccentric, long-period, low-mass eclipsing binary.