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相关论文: Exotic populations in Galactic Globular Clusters

200 篇论文

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

Dense stellar clusters are natural sites for the origin and evolution of exotic objects such as relativistic binaries (potential gravitational wave sources), blue stragglers, etc. We investigate the secular dynamics of a binary system…

太阳与恒星天体物理 · 物理学 2019-08-19 Chris Hamilton , Roman R. Rafikov

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

A model for the mass in and around the Local Group previously used to fit redshifts of dwarf galaxies to their distances between 50 kpc and 2.6 Mpc under the condition of small and growing primeval departures from homogeneity is shown to…

星系天体物理 · 物理学 2017-08-16 P. J. E. Peebles

We report the discovery of a variable blue straggler in the core of the globular cluster M5, based on a 12-hour long series of images obtained with the Planetary Camera aboard the Hubble Space Telescope. In addition, we present the light…

天体物理学 · 物理学 2009-10-30 L. Drissen , M. M. Shara

We summarize some observational comparison concerning the features of globular clusters (GCs) population in connection to the evolution of King models. We also make a comparison with some extragalactic GCs systems, in order to underline the…

星系天体物理 · 物理学 2014-05-20 Marco Merafina , Daniele Vitantoni

In this paper, I review some of the basic properties of the pulsar population in globular clusters (GCs) and compare it with the the Galactic disk population. The neutron stars (NSs) in GCs were likely formed - and appear to continue…

星系天体物理 · 物理学 2015-06-11 Paulo C. C. Freire

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…

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

Globular clusters are known to host an unusually large population of millisecond pulsar when compared to the Galactic disk. This is thanks to the high rate of dynamical encounters occurring in the clusters that can create the conditions to…

高能天体物理现象 · 物理学 2021-12-14 F. Abbate

The field of the globular cluster NGC 6362 was monitored between 1995 and 2009 in a search for variable stars. BV light curves were obtained for 69 periodic variables including 34 known RR Lyr stars, 10 known objects of other types and 25…

太阳与恒星天体物理 · 物理学 2015-01-22 J. Kaluzny , I. B. Thompson , M. Rozyczka , W. Pych , W. Narloch

Improved observations of globular clusters are uncovering a large number of radio pulsars and of X-ray sources. The latter include binaries in which a neutron star or a white dwarf accretes matter from a companion, recycled pulsars, and…

天体物理学 · 物理学 2007-05-23 Frank Verbunt

The dynamics of a close binary system of globular clusters is considered. It is shown that the star transfer process from one of the components to the other should lead to the decrease of dimension of the first cluster with simultaneous…

天体物理学 · 物理学 2009-10-31 G. A. Gurzadyan

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

Globular clusters are valuable fossil records of the formation and evolution of their host galaxies. The color distribution of elliptical galaxy globular cluster systems indicates an episodic formation history, consistent with a merger…

天体物理学 · 物理学 2007-05-23 Stephen E. Zepf

Millisecond Pulsars (MSPs) are fast rotating, highly magnetized neutron stars. According to the "canonical recycling scenario", MSPs form in binary systems containing a neutron star which is spun up through mass accretion from the evolving…

太阳与恒星天体物理 · 物理学 2014-05-14 Cristina Pallanca

We have used multi-band high resolution HST WFPC2 and ACS observations combined with wide field ground-based observations to study the blue straggler star (BSS) population in the galactic globular cluster NGC 6388. As in several other…

天体物理学 · 物理学 2009-11-13 E. Dalessandro , B. Lanzoni , F. R. Ferraro , R. T. Rood , A. Milone , G. Piotto , E. Valenti

Globular clusters produce many exotic stars due to a much higher frequency of dynamical interactions in their dense stellar environments. Some of these objects were observed together with several hundred thousands other stars in our MUSE…

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

Globular clusters are collisional systems, meaning that the stars inside them interact on timescales much shorter than the age of the Universe. These frequent interactions transfer energy between stars and set up observable trends that tell…

星系天体物理 · 物理学 2020-03-18 Laura L. Watkins , Roeland P. van der Marel , Andrea Bellini , Mattia Libralato , Jay Anderson