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相关论文: Visual binary stars: data to investigate formation…

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The frequency of planets in binaries is an important issue in the field of extrasolar planet studies, because of its relevance in estimating of the global planet population of our Galaxy and the clues it can give to our understanding of…

天体物理学 · 物理学 2009-11-13 M. Bonavita , S. Desidera

The unparalleled photometric data obtained by NASA's Kepler Space Telescope has led to an improved understanding of stellar structure and evolution - in particular for solar-like oscillators in this context. Binary stars are fascinating…

Binary stars are common in star clusters and galaxies, but the detailed effects of binary evolution are not taken into account in some colour-magnitude diagram (CMD) studies. This paper studies the CMDs of twelve globular clusters via…

太阳与恒星天体物理 · 物理学 2015-06-12 Zhongmu Li , Caiyan Mao , Ruheng Li , Ruxi Li , Maocai Li

The majority of star formation results in binaries or higher multiple systems, and planets in such systems are constrained to a limited range of orbital parameters in order to remain stable against perturbations from stellar companions.…

地球与行星天体物理 · 物理学 2024-07-22 Billy Quarles , Hareesh Gautham Bhaskar , Gongjie Li

We have developed a general statistical procedure for analysis of 2D and 3D finite patterns, which is applied to the data from recently released Gaia-ESA catalogue DR2. The 2D analysis clearly confirms our former results on the presence of…

天体物理仪器与方法 · 物理学 2019-11-19 Petr Zavada , Karel Píška

The observable spectrum of an unresolved binary star system is a superposition of two single-star spectra. Even without a detectable velocity offset between the two stellar components, the combined spectrum of a binary system is in general…

We report on the results of a survey for radial velocity variability in a heterogeneous sample of very low-mass stars and brown dwarfs. One distinguishing characteristic of the survey is its timespan, which allows an overlap between…

天体物理学 · 物理学 2008-11-26 Gibor Basri , Ansgar Reiners

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

Massive binaries are crucial laboratories that allow us to investigate processes occurring in quite extreme conditions, such as particle acceleration, high-energy emission, or even dust formation. All these processes are intimately…

太阳与恒星天体物理 · 物理学 2009-04-21 M. De Becker

The present dynamical configuration of planets in binary star systems may not reflect their formation process since the binary orbit may have changed in the past after the planet formation process was completed. An observed binary system…

天体物理学 · 物理学 2009-11-13 F. Marzari , M. Barbieri

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…

地球与行星天体物理 · 物理学 2025-08-13 Philippe Thebault , Danilo Bonanni

In an effort to better understand the details of the stellar structure and evolution of metal poor stars, the Gemini North telescope was used on two occasions to take speckle imaging data of a sample of known spectroscopic binary stars and…

Symbiotic stars are long-period interacting binary systems in which an evolved red giant star transfers material to its much hotter compact companion. Such a composition places them among the most variable stars. In addition to periodic…

天体物理学 · 物理学 2007-05-23 Joanna Mikolajewska

Context. Understanding the formation and evolution of star clusters in the Milky Way requires precise identification of clusters that form binary or multiple systems. Such systems offer valuable insight into the dynamical processes and…

星系天体物理 · 物理学 2025-01-22 Tali Palma , Valeria Coenda , Gustavo Baume , Carlos Feinstein

Recent surveys indicate that planets in binary systems are more abundant than previously thought, which is in agreement with theoretical work on disc dynamics and planet formation in binaries. In order to measure the abundance and physical…

地球与行星天体物理 · 物理学 2020-11-11 J. Hagelberg , N. Engler , C. Fontanive , S. Daemgen , S. P. Quanz , J. Kühn , M. Reggiani , M. Meyer , R. Jayawardhana , V. Kostov

Simulations of binary neutron stars have seen great advances in terms of physical detail and numerical quality. However, the spin of the neutron stars, one of the simplest global parameters of binaries, remains mostly unstudied. We present…

广义相对论与量子宇宙学 · 物理学 2015-04-15 Sebastiano Bernuzzi , Tim Dietrich , Wolfgang Tichy , Bernd Bruegmann

With the advent of large-collecting-area instruments, the number of objects that can be reached by optical long-baseline interferometry is steadily increasing. We present here a few results on massive binary stars, showing the interest of…

太阳与恒星天体物理 · 物理学 2015-06-03 Florentin Millour , Anthony Meilland , Philippe Stee , Olivier Chesneau

Binary stars have been shown to have a substantial impact on the integrated light of stellar populations, particularly at low metallicity and early ages - conditions prevalent in the distant Universe. But the fraction of stars in stellar…

星系天体物理 · 物理学 2020-05-06 E. R. Stanway , A. A. Chrimes , J. J. Eldridge , H. F. Stevance , .

Context. This work is part of a long-term spectroscopic study of a sample of 30 multiple stars with early-type components. In this second paper we present the results of six multiple systems in which new stellar components have been…

太阳与恒星天体物理 · 物理学 2014-09-05 M. E. Veramendi , J. F. González

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…

太阳与恒星天体物理 · 物理学 2017-05-03 Andrei Tokovinin