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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

We investigate the distribution of Blue Straggler stars in the field of three open star clusters. The main purpose is to highlight the crucial role played by general Galactic disk fore-/back-ground field stars, which are often located in…

天体物理学 · 物理学 2009-11-13 G. Carraro , R. A. Vazquez , A. Moitinho

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

We study the post-main sequence evolution of products of collisions between main sequence stars (blue stragglers), with particular interest paid to the horizontal branch and asymptotic giant branch phases. We found that the blue straggler…

天体物理学 · 物理学 2011-02-11 Alison Sills , Amanda Karakas , John Lattanzio

The dynamical evolution of globular clusters is theoretically described by a series of well known events typical of N-body systems. Still, the identification of observational signatures able to empirically describe the stage of dynamical…

太阳与恒星天体物理 · 物理学 2023-02-01 Giacomo Beccari , Mario Cadelano , Emanuele Dalessandro

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

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

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

Building on the recent release of a new \emph{Gaia}-based blue straggler star catalog in Galactic open star clusters (OCs), we explored the properties of these stars in a cluster sample spanning a wide range in fundamental parameters. We…

太阳与恒星天体物理 · 物理学 2024-02-26 M. J. Rain , M. S. Pera , G. Perren , O. Benvenuto , J. Panei , A. de Vito , G. Carraro , S. Villanova

We use smoothed-particle hydrodynamics to examine differences between direct collisions of single stars and binary star mergers in their roles as possible blue straggler star formation mechanisms. We find in all cases that core helium in…

天体物理学 · 物理学 2009-10-28 Eric L. Sandquist , Michael Bolte , Lars Hernquist

To probe the nature of stellar evolution in dense environments, we study the dense core of the globular cluster Messier 13 using pre-refurbishment Planetary Camera-I images obtained with the Hubble Space Telescope. We find 15 blue straggler…

天体物理学 · 物理学 2009-10-28 Randi L. Cohen , Puragra Guhathakurta , Brian Yanny , Donald P. Schneider , John N. Bahcall

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

We report the results of new SPH calculations of parabolic collisions between two main-sequence stars in a globular cluster. Such collisions are directly relevant to the formation of blue stragglers. In particular, we consider parent stars…

天体物理学 · 物理学 2009-10-28 J. C. Lombardi , F. A. Rasio , S. L. Shapiro

We continue our exploration of collisionally merged stars in the blue straggler region of the color-magnitude diagram. We report the results of new SPH calculations of parabolic collisions between two main-sequence stars, with the initial…

天体物理学 · 物理学 2012-08-27 Alison Sills , Joshua A. Faber , James C. Lombardi, , Frederic A. Rasio , Aaron Warren

Collisions of main sequence stars occur frequently in dense star clusters. In open and globular clusters, these collisions produce merger remnants that may be observed as blue stragglers. Detailed theoretical models of this process require…

High-resolution {\sl Hubble Space Telescope} imaging observations show that the radial distribution of the field-decontaminated sample of 162 'blue straggler' stars (BSs) in the $11.7^{+0.2}_{-0.1}$ Gyr-old Large Magellanic Cloud cluster…

太阳与恒星天体物理 · 物理学 2015-06-15 Chengyuan Li , Richard de Grijs , Licai Deng , Xiangkun Liu

We show that the X-ray source W31 in the core of the globular cluster 47 Tucanae is physically associated with the bright blue straggler BSS-7. The two sources are astrometrically matched to 0.061\arcsec, with a chance coincidence…

天体物理学 · 物理学 2009-11-13 C. Knigge , R. L. Gilliland , A. Dieball , D. R. Zurek , M. M. Shara , K. S. Long

We examine the blue straggler star (BSS) populations of six old ($\geq$4 Gyr) open clusters: M67, NGC 188, NGC 6791, Berkeley 32, Berkeley 39, and Trumpler 19. We find that 50% of BSSs have color-magnitude diagram (CMD) locations…

太阳与恒星天体物理 · 物理学 2026-05-15 Evan Linck , Robert D. Mathieu

We investigate the evolution of the radial distribution of Blue Straggler Stars through a set of Monte Carlo simulations of star clusters under a variety of initial conditions. We used a novel technique based on the "artificial…

星系天体物理 · 物理学 2018-12-19 A. Sollima , F. R. Ferraro

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