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相关论文: Ecology of Blue Straggler Stars

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Blue straggler stars are the most prominent bright objects in the colour-magnitude diagram of a star cluster that challenges the theory of stellar evolution. Star clusters are the closest counterparts of the theoretical concept of simple…

太阳与恒星天体物理 · 物理学 2015-06-22 Yu Xin , Licai Deng

Blue straggler star (BSS) candidates have been observed in all old dwarf spheroidal galaxies (dSphs), however whether or not they are authentic BSSs or young stars has been a point of debate. To both address this issue and obtain a better…

天体物理学 · 物理学 2009-11-13 M. Mapelli , E. Ripamonti , E. Tolstoy , S. Sigurdsson , M. J. Irwin , G. Battaglia

Blue straggler stars are unique main-sequence stars that appear more luminous, hotter, and therefore younger, than their coeval counterparts. In star clusters, these stars are located above the cluster turn-off in the Hertzsprung-Russell…

太阳与恒星天体物理 · 物理学 2025-01-24 Chen Wang , Taeho Ryu

In this chapter we review the various suggested channels for the formation and evolution of blue straggler stars (BSSs) in different environments and their observational predictions. These include mass transfer during binary stellar…

太阳与恒星天体物理 · 物理学 2015-06-22 Hagai B. Perets

In this chapter I review the recent developments regarding the study of Blue Stragglers (BSS) in dwarf galaxies. The loose density environment of dwarf galaxies resembles that of the Galactic Halo, hence it is natural to compare their…

太阳与恒星天体物理 · 物理学 2015-06-22 Yazan Momany

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…

Blue straggler stars (BSSs) are stars observed to be hotter and bluer than other stars with the same luminosity in their environment. As such they appear to be much younger than the rest of the stellar population. Two main channels have…

太阳与恒星天体物理 · 物理学 2011-02-11 Hagai B. Perets , Daniel C. Fabrycky

Blue straggler stars (BSSs) are brighter and bluer than the main-sequence (MS) turnoff and more massive than MS stars.Two scenarios for their formation have been proposed: collision-induced stellar mergers (COL-BSSs),or mass-transfer in…

星系天体物理 · 物理学 2014-04-29 L. Lovisi

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

By using the high resolution spectrograph FLAMES@VLT we performed the first systematic campaign devoted to measure chemical abundances of blue straggler stars (BSSs). These stars, whose existence is not predicted by the canonical stellar…

星系天体物理 · 物理学 2014-01-17 L. Lovisi

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

Globular clusters are known to host peculiar objects, named Blue Straggler Stars (BSSs), significantly heavier than the normal stellar population. While these stars can be easily identified during their core hydrogen-burning phase, they are…

太阳与恒星天体物理 · 物理学 2016-01-20 F. R. Ferraro , E. Lapenna , A. Mucciarelli , B. Lanzoni , E. Dalessandro , C. Pallanca , D. Massari

Blue stragglers (BSS) are stars whose position in the Color-Magnitude Diagram (CMD) places them above the main sequence turn-off (TO) point of a star cluster. Using data from the core of 47 Tuc in the ultraviolet (UV), we have identified…

太阳与恒星天体物理 · 物理学 2016-10-26 Javiera Parada , Harvey Richer , Jeremy Heyl , Jason Kalirai , Ryan Goldsbury

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

We analyze {\sl Hubble Space Telescope} observations of nine Large Magellanic Cloud star clusters with ages of 1--2 Gyr to search for evolved counterparts of blue straggler stars. Near the red clump regions in the clusters' color--magnitude…

太阳与恒星天体物理 · 物理学 2018-08-29 Chengyuan Li , Licai Deng , Kenji Bekki , Jongsuk Hong , Richard de Grijs , Bi-Qing For

Blue straggler stars (BSS) have been identified in star clusters and in field populations in our own Milky Way galaxy and in its satellite galaxies. They manifest as stars bluer and more luminous than the dominant old population, and…

星系天体物理 · 物理学 2020-04-08 Rosemary F. G. Wyse , Maxwell Moe , Kaitlin M. Kratter

Most stars are members of binaries, and the evolution of a star in a close binary system differs from that of an ioslated star due to the proximity of its companion star. The components in a binary system interact in many ways and binary…

太阳与恒星天体物理 · 物理学 2015-05-14 Z. Han , X. Chen , F. Zhang , Ph. Podsiadlowski

In the context of dwarf spheroidal galaxies it is hard to firmly disentangle a genuine Blue Stragglers (BSS) population from a normal young main (MS) sequence. This difficulty is persistent. For a sample of 9 non-star forming Local Group…

天体物理学 · 物理学 2007-11-07 Y. Momany , E. V. Held , I. Saviane , S. Zaggia , L. Rizzi , M. Gullieuszik

Although the formation of blue straggler stars (BSSs) is routinely attributed to stellar interactions in binary systems, the relative importance of the direct collision and slow(er) stellar coalescence formation channels is still poorly…

太阳与恒星天体物理 · 物理学 2018-11-26 Richard de Grijs , Weijia Sun , Chengyuan Li , Licai Deng

We report the first detections of Blue Straggler Stars (BSS) in the bulge of the Milky Way galaxy. Proper motions from extensive space-based observations along a single sight-line allow us to separate a sufficiently clean and…

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