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相关论文: Blue Stragglers in Galactic Globular Clusters: Pla…

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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

We discuss the main properties of the Galactic globular cluster (GC) blue straggler stars (BSS), as inferred from our new catalog containing nearly 3000 BSS. The catalog has been extracted from the photometrically homogeneous V vs. (B-V)…

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…

Aims: This paper presents a new homogeneous catalogue of blue straggler stars (BSS) in Galactic open clusters. Methods: Photometric data for 216 clusters were collected from the literature and 2782 BSS candidates were extracted from 76 of…

天体物理学 · 物理学 2009-11-11 F. De Marchi , F. De Angeli , G. Piotto , G. Carraro , M. B. Davies

The central regions of six Galactic Globular Clusters (GGCs) (M3, M80, M10, M13, M92 and NGC 288) have been imaged using HST-WFPC2 and the ultraviolet (UV) filters (F255W, F336W). The selected sample covers a large range in both central…

天体物理学 · 物理学 2009-11-07 Francesco R. Ferraro , Alison Sills , Robert T. Rood , Barbara Paltrinieri , Roberto Buonanno

We examine the blue straggler populations of 13 low-luminosity (M_V_t >~ -6) globular clusters and 2 old open clusters. These clusters test blue straggler formation in environments intermediate between higher luminosity (and usually higher…

天体物理学 · 物理学 2009-11-13 Eric L. Sandquist

Blue straggler stars (BSS) are abundantly observed in all Galactic globular clusters (GGC) where data exist. However, observations alone cannot reveal the relative importance of various formation channels or the typical formation times for…

太阳与恒星天体物理 · 物理学 2015-06-15 Sourav Chatterjee , Frederic A. Rasio , Alison Sills , Evert Glebbeek

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

In this paper we report on the most significant results from a statistical analysis of the main properties of globular cluster blue straggler stars (BSS) extracted from the HST snapshot database of photometrically homogeneous CMDs (Piotto…

天体物理学 · 物理学 2007-05-23 Francesca De Angeli , Giampaolo Piotto

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

Recent HST observations of a large sample of globular clusters reveal that every cluster contains between 40 and 400 blue stragglers. The population does not correlate with either stellar collision rate (as would be expected if all blue…

天体物理学 · 物理学 2009-11-10 Melvyn B. Davies , Giampaolo Piotto , Francesca De Angeli

We have analyzed populations of blue straggler stars (BSSs) in 24 Magellanic Cloud star clusters using multi-passband Hubble Space Telescope images. We compiled a homogeneous BSS database, containing both traditional and evolved BSSs. We…

太阳与恒星天体物理 · 物理学 2018-08-08 Weijia Sun , Chengyuan Li , Richard de Grijs , Licai Deng

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

By combining high-resolution HST and wide-field ground based observations, in ultraviolet and optical bands, we study the Blue Stragglers Star (BSS) population of the galactic globular cluster M5 (NGC 5904) from its very central regions up…

天体物理学 · 物理学 2009-06-23 B. Lanzoni , E. Dalessandro , F. R. Ferraro , C. Mancini , G. Beccari , R. T. Rood , M. Mapelli , S. Sigurdsson

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

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

We present new Blue Straggler Star (BSS) catalogs in 38 Milky Way globular clusters (GCs) based on multi-passband and multi-epoch treasury survey data from the Hubble Space Telescope. We measure precise astrometry and relative proper…

太阳与恒星天体物理 · 物理学 2016-11-01 Mirko Simunovic , Thomas H. Puzia

We present the first dynamical study of Blue Straggler Stars (BSSs) in three Galactic globular clusters, NGC\,3201, NGC\,5139 ($\omega$Cen), and NGC\,6218, based on medium-resolution spectroscopy (R 10000) obtained with IMACS. Our BSS…

星系天体物理 · 物理学 2015-06-18 Mirko Simunovic , Thomas H. Puzia

Blue stragglers are anomalously luminous core hydrogen-burning stars formed through mass-transfer in binary/triple systems and stellar collisions. Their physical and evolutionary properties are largely unknown and unconstrained. Here we…

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
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