Results 21 to 30 of about 2,153,296 (418)

Binaries in Globular Clusters [PDF]

open access: yesHighlights of Astronomy, 1998
Binary stars in a globular cluster (hereafter, GC) may be primordial (i.e. formed along with the cluster), or the result of cluster dynamics. “Dynamical” binaries can result from conservative three-body encounters (e.g. Spitzer, 1987) if a third star can carry away enough kinetic energy to leave two others bound, or from dissipative two-body encounters,
McMillan, S. L. W.   +2 more
openaire   +5 more sources

The formation and assembly history of the Milky Way revealed by its globular cluster population [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2018
We use the age–metallicity distribution of 96 Galactic globular clusters (GCs) to infer the formation and assembly history of the Milky Way (MW), culminating in the reconstruction of its merger tree.
J. Kruijssen   +5 more
semanticscholar   +1 more source

The Globular Cluster Systems of Ultra-diffuse Galaxies in the Coma Cluster [PDF]

open access: yesAstrophysical Journal, 2018
Ultra-diffuse galaxies (UDGs) are unusual galaxies with low luminosities, similar to classical dwarf galaxies, but with sizes up to ∼5 larger than expected for their mass.
Sungsoon Lim   +6 more
semanticscholar   +1 more source

Properties of Globular Clusters in Galaxy Clusters: Sensitivity from the Formation and Evolution of Globular Clusters [PDF]

open access: yes, 2022
We investigate the properties of globular clusters in a galaxy cluster, using the particle tagging method with a semi-analytical approach in a cosmological context. We assume globular clusters form from dark matter halo mergers and their metallicity is assigned based on the stellar mass of the host dark matter halos and the formation redshift of GCs ...
arxiv   +1 more source

The Relationship between Globular Cluster Mass, Metallicity, and Light-element Abundance Variations [PDF]

open access: yesAstronomical Journal, 2019
We investigate aluminum abundance variations in the stellar populations of globular clusters using both literature measurements of sodium and aluminum and APOGEE measurements of nitrogen and aluminum abundances.
D. Nataf   +9 more
semanticscholar   +1 more source

NOVAE IN GLOBULAR CLUSTERS [PDF]

open access: yesThe Astrophysical Journal, 2013
13 pages, 14 figures, to appear in ...
Izumi Hachisu, Martin Henze, Mariko Kato
openaire   +3 more sources

Globular cluster star classification: Application to M13 [PDF]

open access: yesSerbian Astronomical Journal, 2013
Starting from recent determination of Fe, O, Na abundances on a restricted sample (N = 67) of halo and thick disk stars, a natural and well motivated selection criterion is defined for the classification globular cluster stars. An application is
Caimmi R.
doaj   +1 more source

A detached stellar-mass black hole candidate in the globular cluster NGC 3201 [PDF]

open access: yes, 2018
As part of our massive spectroscopic survey of 25 Galactic globular clusters with MUSE, we performed multiple epoch observations of NGC 3201 with the aim of constraining the binary fraction. In this cluster, we found one curious star at the main-sequence
B. Giesers   +11 more
semanticscholar   +1 more source

Binary black hole mergers from globular clusters: the impact of globular cluster properties [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2018
The dense environment of globular clusters (GCs) can facilitate the formation of binary black holes (BBHs), some of which can merge with gravitational waves within the age of the Universe.
Jongsuk Hong   +5 more
semanticscholar   +1 more source

Globular cluster candidates within the Fornax Cluster: Intracluster globulars? [PDF]

open access: yesAstronomy & Astrophysics, 2003
We present the results of a search for globular clusters in the surroundings of 15 low surface brightness dwarf galaxies belonging to the Fornax Cluster, which was carried out on CCD images obtained with the C and T1 filters of the Washington photometric system.
Boris Dirsch   +5 more
openaire   +4 more sources

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