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Interacting Binaries consist of a variety of stellar objects in different stages of evolution and those containing accreting compact objects still represent a major challenge to our understanding of not only close binary evolution but also…

Astrophysics · Physics 2009-11-11 B. T. Gaensicke , D. de Martino , T. R. Marsh , C. A. Haswell , C. Knigge , K. S. Long , S. N. Shore

Dynamical interactions that take place between objects in dense stellar systems lead to frequent formation of exotic stellar objects, unusual binaries, and systems of higher multiplicity. They are most important for the formation of…

Solar and Stellar Astrophysics · Physics 2017-06-26 Natalia Ivanova

Accreting compact objects are crucial to understand several important astrophysical phenomena such as Type Ia supernovae, gravitational waves, or X-ray and $\gamma$-ray bursts. In addition, they are natural laboratories to infer fundamental…

High Energy Astrophysical Phenomena · Physics 2025-03-04 Diogo Belloni , Matthias R. Schreiber

It is now clear that central star binarity plays a key role in the formation and evolution of planetary nebulae, with a significant fraction playing host to close-binary central stars which have survived one or more common envelope…

Solar and Stellar Astrophysics · Physics 2018-10-26 David Jones

The effects of binaries on population studies of stars and stellar phenomena have been investigated over the past 3 decades by many research groups. Here we will focus mainly on the work that has been done recently in Brussels and we will…

Astrophysics · Physics 2009-11-10 D. Vanbeveren

Massive stars are among the most important objects in the Universe and many (most?) of them are formed in binaries. A selection of observational and theoretical facts that illustrate the importance of binaries and the evolution of massive…

Solar and Stellar Astrophysics · Physics 2015-05-20 D. Vanbeveren

Ultra-compact X-ray binaries (UCXBs) are a subclass of low-mass X-ray binaries (LMXBs) characterized by ultra-short orbital periods, typically less than $60-80\,$min. They consist of a compact mass-accretor and a hydrogen-poor mass-donor,…

High Energy Astrophysical Phenomena · Physics 2026-03-17 Bo Wang , Dongdong Liu , Yunlang Guo , Hailiang Chen , Wencong Chen , Zhanwen Han

We report on recent progress in our theoretical understanding of X-ray binaries, which has largely been driven by new observations, and illustrate the interplay between theory and observations considering as examples intermediate-mass X-ray…

Astrophysics · Physics 2007-05-23 Philipp Podsiadlowski , Eric Pfahl , Saul Rappaport

It is now clear that a binary evolutionary pathway is responsible for a significant fraction of all planetary nebulae, with some authors even going so far as to claim that binarity may be a near requirement for the formation of an…

Solar and Stellar Astrophysics · Physics 2018-12-11 David Jones

This article reviews the current works on ultra-compact double-degenerate binaries in the presence of magnetic interaction, in particular, unipolar induction. The orbital dynamics and evolution of compact white-dwarf pairs are discussed in…

High Energy Astrophysical Phenomena · Physics 2009-07-22 Kinwah Wu

Ultra-compact binaries (UCBs) are systems containing compact or degenerate stars with orbital periods less than one hour. Tens of millions of UCBs are predicted to exist within theGalaxy emitting gravitational waves (GWs) at mHz…

We first summarize work that has been done on the effects of binaries on theoretical population synthesis of stars and stellar phenomena. Next, we highlight the influence of stellar dynamics in young clusters by discussing a few candidate…

Astrophysics · Physics 2009-11-13 D. Vanbeveren , H. Belkus , J. Van Bever , N. Mennekens

Close-binary central stars of planetary nebulae offer a unique tool with which to study the critical and yet poorly understood common-envelope phase of binary stellar evolution. Furthermore, as the nebula itself is thought to comprise the…

Solar and Stellar Astrophysics · Physics 2024-12-13 David Jones

A binary in which a slightly evolved star starts mass transfer to a neutron star can evolve towards ultra-short orbital periods under the influence of magnetic braking. This is called magnetic capture. We investigate in detail for which…

Astrophysics · Physics 2009-11-10 M. V. van der Sluys , F. Verbunt , O. R. Pols

Ultraluminous X-ray binaries have challenged our assumptions of extreme accretion rates in X-ray binaries, and impact other subfields of astronomy, such as cosmology, gravitational wave sources and supernov{\ae}. Our understanding of ULXs…

High Energy Astrophysical Phenomena · Physics 2024-07-03 Kristen C. Dage , Konstantinos Kovlakas

Binary interactions are commonplace among massive stars, giving rise observed phenomena such as X-ray binaries, stripped stars & supernovae, and gravitational-wave sources. The multiplicity properties of massive stars thus represent a…

Solar and Stellar Astrophysics · Physics 2024-10-22 Tomer Shenar

Within the dynamically cold low inclination portion of the Classical Kuiper Belt, there exists a population of weakly bound binary systems with a number of unusual properties; most notable of which is their extremely wide orbital…

Earth and Planetary Astrophysics · Physics 2022-12-28 Hunter M. Campbell , Lukas R. Stone , Nathan A. Kaib

Stellar astrophysicists are increasingly taking into account the effects of orbiting companions on stellar evolution. New discoveries, many thanks to systematic time-domain surveys, have underlined the role of binary star interactions in a…

Solar and Stellar Astrophysics · Physics 2017-01-18 Orsola De Marco , Robert G. Izzard

Binary interactions lead to the formation of intriguing objects, such as compact binaries, supernovae, gamma ray bursts, X-ray binaries, pulsars, novae, cataclysmic variables, hot subdwarf stars, barium stars, and blue stragglers. To study…

Solar and Stellar Astrophysics · Physics 2020-11-11 Zhanwen Han , Hongwei Ge , Xuefei Chen , Hailiang Chen

Binary stars play a critical role in determining both the dynamical evolution and the observational appearance of globular star clusters. We present a summary of three talks presented at IAU JD15, reviewing the current observational and…

Astrophysics · Physics 2007-05-23 S. L. W. McMillan , C. Pryor , E. S. Phinney
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