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相关论文: Statistical Study of the Blue Straggler Properties…

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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)…

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

We present preliminary results obtained from the comparison of the specific frequencies of Blue Straggler Stars (BSS) detected so far in a sample of 26 Galactic globular clusters. The number of BSS seems to increase almost linearly with…

天体物理学 · 物理学 2011-05-23 F. R. Ferraro , F. Fusi Pecci , M. Bellazzini

This chapter presents an overview of the main observational results obtained to date about Blue Straggler Stars (BSSs) in Galactic Globular Clusters (GCs). The BSS specific frequency, radial distribution, chemical composition and rotational…

太阳与恒星天体物理 · 物理学 2015-06-22 Francesco R. Ferraro , Barbara Lanzoni , Emanuele Dalessandro , Alessio Mucciarelli , Loredana Lovisi

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

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 present early results from a detailed analysis of the BSS population in Galactic GCs based on HST data.Using proper motion cleaning of the color-magnitude diagrams we construct a large catalog of BSSs and study some population…

太阳与恒星天体物理 · 物理学 2015-10-05 Mirko Simunovic , Thomas H. Puzia

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

In this paper I present an overview of the main observational properties of a special class of exotic objects (the so-called Blue Straggler Stars, BSSs) in Galactic Globular Clusters (GCs). The BSS specific frequency and their radial…

星系天体物理 · 物理学 2017-08-23 Francesco R. Ferraro

Blue straggler stars (BSSs) are exotic objects, which, being the results of processes such as mass transfer, mergers, or collisions, are considered key objects in the study of their host clusters' dynamics. While many studies on…

太阳与恒星天体物理 · 物理学 2026-01-14 Lorenzo Briganti , Walter Eduard van Rossem , Andrea Miglio , Angela Bragaglia , Massimiliano Matteuzzi

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 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 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

The core of the Galactic Globular Cluster M3 (NGC 5272) has been observed with the WFPC2 through the filters F255W, F336W, F555W, and F814W. Using these observations along with a thorough reanalysis of earlier catalogs, we have produced a…

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

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

We have used high resolution WFPC2-HST and wide field ground-based observations to construct a catalog of blue straggler stars (BSS) which spans the entire radial extent of the globular cluster NGC 6752. The BSS sample is the most extensive…

天体物理学 · 物理学 2009-11-10 E. Sabbi , F. R. Ferraro , A. Sills , R. T. Rood

Among the most striking feature of blue straggler stars (BSS) is the presence of multiple sequences of BSSs in the colour-magnitude diagrams (CMDs) of several globular clusters. It is often envisaged that such a multiple BSS sequence would…

星系天体物理 · 物理学 2016-06-17 Sambaran Banerjee

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

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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