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Related papers: Pairing mechanisms for binary stars

200 papers

There exist discrepancies in measurements of the number and evolution of galaxy pairs. The pair fraction appears to be sensitive to both the criteria used to select pair fraction and the methods used to analyze survey data. This paper…

Astrophysics of Galaxies · Physics 2020-10-07 Philip J. Grylls , F. Shankar , C. Conselice

Almost all young stars are found in multiple systems. This suggests that protostellar cores almost always fragment into multiple objects. The observed properties of multiple systems such as their separation distribution and mass ratios…

Astrophysics · Physics 2007-05-23 S. P. Goodwin , P. Kroupa , A. Goodman , A. Burkert

The statistical properties of planets in binaries were investigated. Any difference to planets orbiting single stars can shed light on the formation and evolution of planetary systems. As planets were found around components of binaries…

Astrophysics · Physics 2009-11-11 S. Desidera , M. Barbieri

Red giants are increasingly used as stellar population tracers due to their well-understood evolution and the availability of asteroseismic observables. However, stellar binarity can alter observable properties and introduce strong biases.…

Solar and Stellar Astrophysics · Physics 2026-02-02 Paul G. Beck

Estimating the effect binarity can have on planet-formation is of crucial importance, as almost half of field stars reside in multiple systems. One effective way to assess this effect is to get an accurate picture of the population of…

Earth and Planetary Astrophysics · Physics 2025-08-13 Philippe Thebault , Danilo Bonanni

We study the formation of massive Population III binary stars using a newly developed radiation hydrodynamics code with the adaptive mesh refinement and adaptive ray-tracing methods. We follow the evolution of a typical primordial…

Astrophysics of Galaxies · Physics 2020-06-16 Kazuyuki Sugimura , Tomoaki Matsumoto , Takashi Hosokawa , Shingo Hirano , Kazuyuki Omukai

The stability criteria of rapid mass transfer and common-envelope evolution are fundamental in binary star evolution. They determine the mass, mass ratio, and orbital distribution of many important systems, such as X-ray binaries, type Ia…

Solar and Stellar Astrophysics · Physics 2024-11-27 Hongwei Ge , Zhanwen Han

Binary and multiple stellar systems are numerous in our solar neighborhood with 80 per cent of the solar-type stars being members of systems with high order multiplicity. The Contact Binaries Towards Merging (CoBiToM) Project is a programme…

Solar and Stellar Astrophysics · Physics 2021-02-10 K. D. Gazeas , G. A. Loukaidou , P. G. Niarchos , S. Palafouta , D. Athanasopoulos , A. Liakos , S. Zola , A. Essam , P. Hakala

The formation and evolution of binary stars is a critical component of several fields in astronomy. The most numerous sources for gravitational wave observatories are inspiraling and/or merging compact binaries, while binary stars are…

Binaries have played a crucial role many times in the history of modern astronomy and are doing so again in the rapidly evolving exploration of the Kuiper Belt. The large fraction of transneptunian objects that are binary or multiple, 48…

Stars are commonly formed in binary systems, which provide a natural laboratory for studying planet formation in extreme conditions. In our first paper (Paper I) of a series Xie et al. (2011), we have shown that the intermediate stage -…

Earth and Planetary Astrophysics · Physics 2018-07-25 Yapeng Zhang , Qingqin Li , Ji-Wei Xie , Ji-Lin Zhou , Hui-Gen Liu , Hui Zhang

Black holes in binary star systems are vital for understanding the process of pr oducing gravitational wave sources, understanding how supernovae work, and for p roviding fossil evidence for the high mass stars from earlier in the Universe.…

Wide gravitationally bound pairs of stars can be formed from adjacent prestellar cores that happen to move slowly enough relative to each other. These binaries are remnants of the primordial clustering. It is shown that the expected…

Solar and Stellar Astrophysics · Physics 2017-05-03 Andrei Tokovinin

In this paper we explore the effects that the presence of a fraction of binary stars has in the determination of a star cluster mass via the virial theorem. To reach this aim in an accurate and consistent way, we run a set of simulations…

Solar and Stellar Astrophysics · Physics 2020-07-01 Sara Rastello , Giovanni Carraro , Roberto Capuzzo-Dolcetta

Binary stars are present in all stellar systems, yet their role is far from being fully understood. We investigate the effect of unresolved binaries in the derivation of open clusters' mass by star counts. We start from the luminosity…

Solar and Stellar Astrophysics · Physics 2019-04-10 Olga I. Borodina , Anton F. Seleznev , Giovanni Carraro , Vladimir M. Danilov

Small planets ($R_{p} \leq 4 R_{\oplus}$) are divided into rocky super-Earths and gaseous sub-Neptunes separated by a radius gap, but the mechanisms that produce these distinct planet populations remain unclear. Binary stars are the only…

Most of massive stars form in binary or higher-order systems in clumpy, sub-structured clusters. In the very first phases of their life, these stars are expected to interact with the surrounding environment, before being released to the…

Understanding the galaxy in which we live is one of the great intellectual challenges facing modern science. With the advent of high quality observational data, the chemical evolution modeling of our galaxy has been the subject of numerous…

Astrophysics · Physics 2009-11-10 Erwin De Donder , Dany Vanbeveren

Binarity among stellar clusters in galaxy is such a reality which has been realized for a long time, but still hides several questions and problems to be solved. Some of binary star clusters are formed by close encounter, but the others are…

Astrophysics of Galaxies · Physics 2015-06-16 Rhorom Priyatikanto , M. Ikbal Arifyanto , Hesti R. T. Wulandari

We now know that a large number of stars are born in multiple systems. Additionally, more than 70% of massive stars are found in close binary systems, meaning that they will interact over the course of their lifetime. This has strong…

Solar and Stellar Astrophysics · Physics 2020-01-31 Heloise F. Stevance , J. J. Eldridge , Elizabeth Stanway