1 code implementation • 16 Nov 2018 • Andrew W. Mann, Trent Dupuy, Adam L. Kraus, Eric Gaidos, Megan Ansdell, Michael Ireland, Aaron C. Rizzuto, Chao-Ling Hung, Jason Dittmann, Samuel Factor, Gregory Feiden, Raquel A. Martinez, Dary Ruiz-Rodriguez, Pa Chia Thao
The result can be used to determine masses of single stars with a precision of 2-3%, which we confirm by a comparison to dynamical masses from the literature.
Solar and Stellar Astrophysics
