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相关论文: Binary origin of blue straggler stars in Galactic …

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Blue straggler stars are exotic objects present in all stellar environments whose nature and formation channels are still partially unclear. They seem to be particularly abundant in open clusters (OCs), thus offering a unique chance to…

太阳与恒星天体物理 · 物理学 2021-06-09 M. J. Rain , J. Ahumada , G. Carraro

Blue stragglers in globular clusters are abnormally massive stars that should have evolved off the stellar main sequence long ago. There are two known processes that can create these objects: direct stellar collisions and binary evolution.…

太阳与恒星天体物理 · 物理学 2009-11-13 Christian Knigge , Nathan Leigh , Alison Sills

Two blue-straggler sequences discovered in globular cluster M30 provide a strong constraint on the formation mechanisms of blue stragglers. We study the formation of the blue-straggler binaries through binary evolution, and find that binary…

太阳与恒星天体物理 · 物理学 2017-11-15 Dengkai Jiang , Xuefei Chen , Lifang Li , Zhanwen Han

(abridged) We use newly available empirical binary fractions for globular clusters to carry out a direct test of the binary evolution hypothesis, and of collisional channels that involve binary stars. More specifically, using the previously…

太阳与恒星天体物理 · 物理学 2015-06-11 Nathan Leigh , Christian Knigge , Alison Sills , Hagai Perets , Ata Sarajedini , Evert Glebbeek

Context. Blue Stragglers Stars (BSSs) are thought to form in globular clusters by two main formation channels: i) mergers induced by stellar collisions and ii) coalescence or mass-transfer between companions in binary systems. The detailed…

天体物理学 · 物理学 2009-11-13 A. Sollima , B. Lanzoni , G. Beccari , F. R. Ferraro , F. Fusi Pecci

Blue stragglers are anomalously massive core hydrogen-burning stars that, according to the theory of single star evolution, should not exist. They are suspected to form in mass-enhancement processes, involving binary evolution or stellar…

Stellar rotation is a fundamental ingredient in shaping the evolution of stars and it can also be used to trace past stellar interactions. Yet, systematic studies of stellar rotation in large samples of stars belonging to different…

Context. The study of blue straggler stars (BSS) provides insight into the mechanisms of stellar mass exchange during binary stellar evolution and the complex gravitational interactions within dense stellar systems. In combination, they…

太阳与恒星天体物理 · 物理学 2025-07-16 Francisco F. Carrasco-Varela , Prasanta K. Nayak , Thomas H. Puzia

Binary stars play a crucial role in our understanding of the formation and evolution of star clusters and their stellar populations. We use Gaia Data Release 3 to homogeneously analyze 78 Galactic open clusters and the unresolved binary…

We present an analytic model for blue straggler formation in globular clusters. We assume that blue stragglers are formed only through stellar collisions and binary star evolution, and compare our predictions to observed blue straggler…

太阳与恒星天体物理 · 物理学 2015-05-28 Nathan Leigh , Alison Sills , Christian Knigge

In this paper, we systematically studied blue stragglers produced from primordial binary evolution via a binary population synthesis approach, and examined their contribution to the integrated spectral energy distributions of the host…

太阳与恒星天体物理 · 物理学 2009-11-13 Xuefei Chen , Zhanwen Han

Context. Origin and evolution of blue stragglers in globular clusters is still a matter of debate. Aims. The aim of the present investigation is to reproduce the evolutionary history of four binary blue stragglers in four different…

太阳与恒星天体物理 · 物理学 2017-01-11 K. Stepien , A. A. Pamyatnykh , M. Rozyczka

Blue straggler stars present as secure members in the Galactic open clusters form a major challenge to the conventional picture of evolutionary population synthesis based on the stellar evolution theory of single stars, as illustrated in…

天体物理学 · 物理学 2011-02-11 Y. Xin , L. Deng , Z. Han

The high-precision {\it Gaia} data release 3 (DR3) enables the discovery of numerous open clusters in the Milky Way, providing an excellent opportunity to search for blue straggler stars in open clusters and investigate their formation and…

太阳与恒星天体物理 · 物理学 2025-11-11 Songmei Qin , Jing Zhong , Friedrich Anders , Lola Balaguer-Núñez , Chunyan Li , Yueyue Jiang , Guimei Liu , Tong Tang , Li Chen

Blue Stragglers are stars located in an unexpected region of the color-magnitude diagram of a stellar population, as they appear bluer and more luminous than the stars in the turnoff region. They are ubiquitous, since they have been found…

太阳与恒星天体物理 · 物理学 2020-01-29 M. J. Rain , G. Carraro , J. A. Ahumada , S. Villanova , H. Boffin , L. Monaco , G. Beccari

Blue straggler stars (BSSs) are the most massive stars in a cluster formed via binary or higher-order stellar interactions. Though the exact nature of such formation scenarios is difficult to pin down, we provide observational constraints…

太阳与恒星天体物理 · 物理学 2021-08-18 Vikrant Jadhav , Annapurni Subramaniam

Binary systems can evolve into immensely different exotic systems such as blue straggle stars (BSSs), yellow straggler stars, cataclysmic variables, type Ia supernovae depending on their initial mass, the orbital parameters and evolution.…

太阳与恒星天体物理 · 物理学 2022-07-11 Vikrant V. Jadhav

Combination of high-precision photometry and spectroscopy allows the detailed study of the upper main sequence in open clusters. We are carrying out a comprehensive study of a number of clusters containing Be stars in order to evaluate the…

天体物理学 · 物理学 2007-05-23 Amparo Marco , Ignacio Negueruela , Christian Motch

We identified blue straggler stars (BSSs) in 53 open clusters utilizing data from Gaia DR3. Most of these clusters are situated in the outer regions of the Galactic disc, encompassing structures such as the warp and the Outer arm. We…

太阳与恒星天体物理 · 物理学 2025-02-27 Qian Cui , Zhihong He , Shunhong Deng , Liming Peng , Chunyan Li , Yangping Luo , Kun Wang

The fraction of binary stars is an important ingredient to interpret globular cluster dynamical evolution and their stellar population. We investigate the properties of main-sequence binaries measured in a uniform photometric sample of 59…

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