A 2+1+1 quadruple star system containing the most eccentric, low-mass, short-period, eclipsing binary known

MLA

Han, E., et al. A 2+1+1 Quadruple Star System Containing the Most Eccentric, Low-Mass, Short-Period, Eclipsing Binary Known. 2021. EBSCOhost, https://doi.org/10.1093/mnras/stab3507.

APA

Han, E., Rappaport, S. A., Vanderburg, A., Tofflemire, B. M., Borkovits, T., Schwengeler, H. M., Zasche, P., Krolikowski, D. M., Muirhead, P. S., Kristiansen, M. H., Terentev, I. A., Omohundro, M., Gagliano, R., Jacobs, T., & LaCourse, D. (2021). A 2+1+1 quadruple star system containing the most eccentric, low-mass, short-period, eclipsing binary known. https://doi.org/10.1093/mnras/stab3507

Chicago

Han, E., S. A. Rappaport, A. Vanderburg, B. M. Tofflemire, T. Borkovits, H. M. Schwengeler, P. Zasche, et al. 2021. “A 2+1+1 Quadruple Star System Containing the Most Eccentric, Low-Mass, Short-Period, Eclipsing Binary Known.” doi:10.1093/mnras/stab3507.