Massive binaries as the source of abundance anomalies in globular clusters

SE De Mink, OR Pols, N Langer, RG Izzard - Astronomy & Astrophysics, 2009 - aanda.org
Abundance anomalies observed in globular cluster stars indicate pollution with material
processed by hydrogen burning. Two main sources have been suggested: asymptotic giant …

The Tarantula Massive Binary Monitoring-VI. Characterisation of hidden companions in 51 single-lined O-type binaries: A flat mass-ratio distribution and black-hole …

T Shenar, H Sana, L Mahy, JM Apellániz… - Astronomy & …, 2022 - aanda.org
Context. Massive binaries hosting a black hole (OB+ BH) represent a critical phase in the
production of BH mergers in the context of binary evolution. In spite of this, such systems …

Taking the measure of the universe: precision astrometry with SIM PlanetQuest

SC Unwin, M Shao, AM Tanner, RJ Allen… - Publications of the …, 2008 - iopscience.iop.org
Precision astrometry at microarcsecond accuracy has applications for a wide range of
astrophysical problems. This paper is a study of the science questions that can be …

First resolved images of the eclipsing and interacting binary β Lyrae

M Zhao, D Gies, JD Monnier, N Thureau… - The Astrophysical …, 2008 - iopscience.iop.org
We present the first resolved images of the eclipsing binary β Lyrae, obtained with the
CHARA Array interferometer and the MIRC combiner in the H band. The images clearly …

Non-conservative evolution in Algols: where is the matter?

R Deschamps, K Braun, A Jorissen, L Siess… - Astronomy & …, 2015 - aanda.org
Context. There is indirect evidence of non-conservative evolutions in Algols. However, the
systemic mass-loss rate is poorly constrained by observations and generally set as a free …

Close Binary Perspectives

RE Wilson - Galaxies, 2020 - mdpi.com
Development of analytic binary star models is discussed in historical and on-going
perspective, beginning with an overview of paradigm shifts, the merits of direct (rectification …

Morphology of the interaction between the stream and cool accretion disk in a semidetached binary system

DV Bisikalo, AA Boyarchuk, PV Kaigorodov… - Astronomy Reports, 2003 - Springer
We analyze heating and cooling processes in accretion disks in binaries. For realistic
parameters of the accretion disks in close binaries (̇ M ≃ 10^-12-10^ 7 M_ ⊙/yr and α⋍ …

The structure of cool accretion disks in semidetached binaries

DV Bisikalo, AA Boyarchuk, PV Kaigorodov… - Astronomy reports, 2004 - Springer
We present a qualitative analysis of possible changes in the structure of accretion disks that
occur in the transition from hot to cool disks. We suggest that an additional spiral-density …

On the accretion disc and evolutionary stage of β Lyrae

RE Mennickent, G Djurašević - Monthly Notices of the Royal …, 2013 - academic.oup.com
We modelled the V-band light curve of β Lyrae (Lyr) with two stellar components plus an
optically thick accretion disc around the gainer assuming a semidetached configuration. We …

The ever challenging emission‐line binary β Lyrae

P Harmanec - Astronomische Nachrichten: Astronomical Notes, 2002 - Wiley Online Library
A brief history of investigations of Lyr, an emission‐line binary and one of the first ever
discovered Be stars is presented. A rather fast progress in the understanding of this …