activity
20012024
most citedAstrophysics of Young Star Binaries

166 citations · 708 across the 10 of their papers we have counts for

collaborators

9 papers

astro-ph.EP2024

Sites of Planet Formation in Binary Systems. I. Evidence for Disk-Orbit Alignment in the Close Binary FO Tau

Benjamin M. Tofflemire, Lisa Prato, Adam L. Kraus +8

Close binary systems present challenges to planet formation. As binary separations decrease, so too do the occurrence rates of protoplanetary disks in young systems and planets in…

astro-ph.SR2020★ 16 cited

Orbital Motion, Variability, and Masses in the T Tauri Triple System

G. H. Schaefer, Tracy L. Beck, L. Prato +1

We present results from adaptive optics imaging of the T Tauri triple system obtained at the Keck and Gemini Observatories in 2015-2019. We fit the orbital motion of T Tau Sb relat…

astro-ph.SR2017★ 5 cited

Science cases for a visible interferometer

Philippe Stee, France Allard, Myriam Benisty +54

High spatial resolution is the key for the understanding various astrophysical phenomena. But even with the future E-ELT, single dish instruments are limited to a spatial resolutio…

astro-ph.SR2014★ 83 cited

The masses of young stars: CN as a probe of dynamical masses

S. Guilloteau, M. Simon, V. Piétu +4

Aims: We attempt to determine the masses of single or multiple young T Tauri and HAeBe stars from the rotation of their Keplerian disks. Methods:We used the IRAM PdBI interferomete…

astro-ph.SR2014★ 59 cited

Orbital Motion in Pre-Main Sequence Binaries

G. H. Schaefer, L. Prato, M. Simon +1

We present results from our ongoing program to map the visual orbits of pre-main sequence binaries in the Taurus star forming region using adaptive optics imaging at the Keck Obser…

astro-ph2006★ 53 cited

Dynamical Mass Estimates for Incomplete Orbits: Young Multiple Stars in Taurus and Ophiuchus

G. H. Schaefer, M. Simon, T. L. Beck +2

We present recent measurements of the orbital motion in the binaries, DF Tau and ZZ Tau, and in the triples, Elias 12, T Tau, and V853 Oph. We observed these systems with the Fine…