collaborators

5 papers

astro-ph.SR2025

Orbital and Physical Properties of the Pleiades Binary 27 Tau (Atlas)

G. Torres, A. Tkachenko, K. Pavlovski +12

We report new spectroscopic and interferometric observations of the Pleiades binary star Atlas, which played an important role nearly three decades ago in settling the debate over…

astro-ph.SR2025

Precise Age For The Binary HD 21278 In The Young Alpha Persei Cluster

Christopher A. Danner, Eric L. Sandquist, Gail H. Schaefer +14

We present a study of the double-lined spectroscopic binary HD 21278 that contains one of the brightest main sequence stars in the young Persei open cluster. We analyzed new sp…

astro-ph.SR2025

Spatially resolved centrifugal magnetosphere caught in motion around the secondary component of Oph A

R. Klement, M. E. Shultz, Th. Rivinius

The recently discovered spectroscopic binary Oph A is a rare magnetic hot binary system composed of two early B-type stars, comprising a non-magnetic primary (Aa) and a slightl…

astro-ph.SR2025

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions

Thibault Lechien, Selma E. de Mink, Ruggero Valli +5

Binary stars and their interactions shape the formation of compact binaries, supernovae, and gravitational wave sources. The efficiency of mass transfer - the fraction of mass reta…

astro-ph.SR2025

VLTI/GRAVITY enables the determination of the first dynamical masses of a classical Be + stripped and bloated pre-subdwarf binary

R. Klement, Th. Rivinius, D. Baade +7

HR~6819 is the first post-mass transfer binary system composed of a classical Be star and a bloated pre-subdwarf stripped star directly confirmed by interferometry. While the Be st…