321 citations · 1.6k across the 15 of their papers we have counts for
15 papers
Dissecting the Quadruple Binary Hyad vA 351 -- Masses for three M Dwarfs and a White Dwarf
G. Fritz Benedict, Otto G. Franz, Elliott P. Horch +8
We extend results first announced by Franz et al. (1998), that identified vA 351 = H346 in the Hyades as a multiple star system containing a white dwarf. With Hubble Space Telescop…
Surveying the Bright Stars by Optical Interferometry I: A Search for Multiplicity Among Stars of Spectral Types F - K
Donald Hutter, Robert Zavala, Christopher Tycner +5
We present the first results from an ongoing survey for multiplicity among the bright stars using the Navy Precision Optical Interferometer (NPOI). We first present a summary of NP…
The Solar Neighborhood XXXVII: The Mass-Luminosity Relation for Main Sequence M Dwarfs
G. F. Benedict, T. J. Henry, O. G. Franz +8
We present a Mass-Luminosity Relation (MLR) for red dwarfs spanning a range of masses from 0.62 Msun to the end of the stellar main sequence at 0.08 Msun. The relation is based on…
Cool Subdwarf Investigations III: Dynamical Masses of Low Metallicity Subdwarfs
Wei-Chun Jao, Ed Nelan, Todd Henry +2
We report dynamical mass measurements for the components of the previously known double-lined spectroscopic subdwarfs G 006-026 B and C using the Fine Guidance Sensors (FGS) on the…
The Highly Eccentric Pre-Main Sequence Spectroscopic Binary RX J0529.3+1210
G. N. Mace, L. Prato, L. H. Wasserman +3
The young system RX J0529.3+1210 was initially identified as a single-lined spectroscopic binary. Using high-resolution infrared spectra, acquired with NIRSPEC on Keck II, we measu…
Optical interferometric observations of Theta 1 Orionis C from NPOI and implications for the system orbit
J. Patience, R. T. Zavala, L. Prato +5
With the Navy Prototype Optical Interferometer (NPOI), the binary system Theta 1 Orionis C, the most massive member of the Trapezium, was spatially resolved over a time period exte…