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Strong encounters between single stars and binaries play a pivotal role in the evolution of star clusters. Such encounters can also dramatically modify the orbital parameters of binaries, exchange partners in and out of binaries, and are a…

太阳与恒星天体物理 · 物理学 2015-08-06 Aaron M. Geller , Nathan W. C. Leigh

Characterization of the binary fractions in star clusters is of fundamental importance for many fields in astrophysics. Observations indicate that the majority of stars are found in binary systems, while most stars with masses greater than…

太阳与恒星天体物理 · 物理学 2015-10-02 Richard de Grijs , Chengyuan Li , Aaron M. Geller

This chapter reviews the dynamical processes in young stellar clusters. The accretion of gas by individual stars affects the dynamics of the cluster, and the masses of the stars. Dynamical mass segregation cannot explain the degree of mass…

天体物理学 · 物理学 2007-05-23 Ian Bonnell , Pavel Kroupa

In dense stellar systems, frequent dynamical interactions between binaries lead to the formation of multiple systems. In this contribution we discuss the dynamical formation of hierarchically stable triples: the formation rate, main…

天体物理学 · 物理学 2009-09-29 Natalia Ivanova

So far, stellar population studies have mainly focused on the evolution of single and binary stars. Recent observations show that triple and higher order multiple star systems are common, especially among massive stars. Introducing…

太阳与恒星天体物理 · 物理学 2023-06-19 F. Kummer , S. Toonen , A. de Koter

(abridged) This thesis presents theoretical and statistical techniques broadly related to systems of dynamically-interacting particles composed of several different types of populations. They are applied to observations of dense star…

太阳与恒星天体物理 · 物理学 2011-08-04 Nathan Leigh

The young star clusters we observe today are the building blocks of a new generation of stars and planets in our Galaxy and beyond. Despite their fundamental role we still lack knowledge about the conditions under which star clusters form…

星系天体物理 · 物理学 2015-03-19 C. Olczak , R. Spurzem , Th. Henning , T. Kaczmarek , S. Pfalzner , S. Harfst , S. Portegies Zwart

We review recent work that investigates the formation of stellar clusters, ranging in scale from globular clusters through open clusters to the small scale aggregates of stars observed in T associations. In all cases, recent advances in…

天体物理学 · 物理学 2007-05-23 Cathie J. Clarke , Ian A. Bonnell , Lynne A. Hillenbrand

The preponderance of binary systems in all known stellar populations makes them exciting dynamical agents for research on topics as varied as star formation, star-cluster dynamics and the interiors of young and old stars. Today we know that…

天体物理学 · 物理学 2007-05-23 Pavel Kroupa

Triple stellar systems, consisting of three gravitationally bound stars, play a fundamental role in a wide array of astrophysical processes, from stellar evolution to the formation of exotic objects and gravitational wave sources. This…

太阳与恒星天体物理 · 物理学 2025-08-26 Hagai B. Perets

Recent radial velocity and transit data discovered $\sim 100$ planets in binary or triple stellar systems out of the entire population of a few thousand known planets. Stellar companions are expected to strongly influence both the formation…

地球与行星天体物理 · 物理学 2018-12-05 Giacomo Fragione , Abraham Loeb , Idan Ginsburg

Massive stars are known to have a high multiplicity, with examples of higher order multiples among the nearest and best studied objects. In this paper we study hierarchical multiple systems (an inner binary as a component of a wider binary)…

太阳与恒星天体物理 · 物理学 2013-01-30 Nickolas Moeckel , Ian A. Bonnell

Close encounters between stars in star forming regions are important as they can perturb or destroy protoplanetary discs, young planetary systems, and stellar multiple systems. We simulate simple, viralised, equal-mass $N$-body star…

星系天体物理 · 物理学 2023-04-26 Krisada Rawiraswattana , Simon P. Goodwin

Around the turn of the last century, star clusters of all kinds were considered "simple" stellar populations. Over the past decade, this situation has changed dramatically. At the same time, star clusters are among the brightest stellar…

太阳与恒星天体物理 · 物理学 2018-01-17 Richard de Grijs , Chengyuan Li

The stars that populate the solar neighbourhood were formed in stellar clusters. Through N-body simulations of these clusters, we measure the rate of close encounters between stars. By monitoring the interaction histories of each star, we…

This review concentrates almost entirely on globular star clusters. It emphasises the increasing realisation that few of the traditional problems of star cluster astronomy can be studied in isolation: the influence of the Galaxy affects…

天体物理学 · 物理学 2016-01-27 Douglas C. Heggie

Stars are mostly found in binary and multiple systems, as at least 50% of all solar-like stars have companions - a fraction that goes up to 100% for the most massive stars. Moreover, a large fraction of them will interact in some way or…

太阳与恒星天体物理 · 物理学 2024-11-28 Henri M. J. Boffin , David Jones

Multiple systems play an important role in the evolution of star clusters. First we discuss several formation mechanisms which depend on the presence of binaries, either primordial or of dynamical origin. Hierarchical configurations are…

天体物理学 · 物理学 2007-05-23 Sverre J. Aarseth , Rosemary A. Mardling

Close, compact, hierarchical, multiple stellar systems, i.e., multiples having an outer orbital period from months to a few years, comprise a small, but continuously growing group of the triple and multiple star zoo. Many of them consist of…

太阳与恒星天体物理 · 物理学 2022-01-05 Tamás Borkovits

The presence of a nearby companion alters the evolution of massive stars in binary systems, leading to phenomena such as stellar mergers, X-ray binaries and gamma-ray bursts. Unambiguous constraints on the fraction of massive stars affected…

太阳与恒星天体物理 · 物理学 2012-07-30 H. Sana , S. E. de Mink , A. de Koter , N. Langer , C. J. Evans , M. Gieles , E. Gosset , R. G. Izzard , J. -B. Le Bouquin , F. R. N. Schneider
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