activity
20042023
most citedA naked-eye triple system with a nonaccreting black hole in the inner binary

98 citations · 353 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.EP2023★ 8 cited

Three-dimensional orbit of AC Her determined: Binary-induced truncation cannot explain the large cavity in this post-AGB transition disk

Narsireddy Anugu, Jacques Kluska, Tyler Gardner +17

Some evolved binaries, namely post-asymptotic giant branch binaries, are surrounded by stable and massive circumbinary disks similar to protoplanetary disks found around young star…

astro-ph.SR2023★ 5 cited

Precise Age for the Binary Star System 12 Com in the Coma Berenices Cluster

Rex Lam, Eric L. Sandquist, Gail H. Schaefer +11

We present measurements of the interferometrically-resolved binary star system 12 Com and the single giant star 31 Com in the cluster Coma Berenices. 12 Com is a double-lined spect…

astro-ph.SR2022★ 26 cited

Gamma Cas Stars as Be + White Dwarf Binary Systems

Douglas Gies, Luqian Wang, Robert Klement

The origin of the bright and hard X-ray emission flux among the gamma Cas subgroup of B-emission line (Be) stars may be caused by gas accretion onto an orbiting white dwarf (WD) co…

astro-ph.SR2022★ 9 cited

The Orbits and Dynamical Masses of the Castor System

Guillermo Torres, Gail H. Schaefer, John D. Monnier +12

Castor is a system of six stars in which the two brighter objects, Castor A and B, revolve around each other every 450 yr and are both short-period spectroscopic binaries. Th…

astro-ph.SR2022★ 11 cited

The Interferometric Binary Epsilon Cancri in Praesepe: Precise Masses and Age

Leslie M. Morales, Eric L. Sandquist, Gail H. Schaefer +16

We observe the brightest member of the Praesepe cluster, Epsilon Cancri, to precisely measure the characteristics of the stars in this binary system, en route to a new measurement…

astro-ph.SR2021★ 9 cited

The Transformative Journey of HD 93521

Douglas R. Gies, Katherine Shepard, Peter Wysocki +1

HD 93521 is a massive, rapidly rotating star that is located about 1 kpc above the Galactic disk, and the evolutionary age for its estimated mass is much less than the time-of-flig…