Results 111 to 120 of about 2,000,138 (297)

Globular cluster formation in the context of galaxy formation and evolution [PDF]

open access: yes, 2014
The formation of globular clusters (GCs) remains one of the main unsolved problems in star and galaxy formation. The past decades have seen important progress in constraining the physics of GC formation from a variety of directions.
J. M. Diederik Kruijssen
semanticscholar   +1 more source

Near-Infrared Photometry of Metal Rich Globular Cluster M71 [PDF]

open access: yesJournal of Astronomy and Space Sciences, 1997
We have carried out JK near-infrared photometry for the central region of the metal rich globular cluster M71, whose(K, J - K) color-magnitude diagram is presented here. Using two independent methods we derive the distance modulus to M71, 12.89 and 12.86
Jae-Mann Kyeong   +2 more
doaj  

Internal Kinematics and Structure of the Bulge Globular Cluster NGC 6569

open access: yesThe Astrophysical Journal, 2023
In the context of a project aimed at characterizing the properties of star clusters in the Galactic bulge, here we present the determination of the internal kinematics and structure of the massive globular cluster NGC 6569.
Cristina Pallanca   +10 more
doaj   +1 more source

A CATALOG OF GLOBULAR CLUSTER SYSTEMS: WHAT DETERMINES THE SIZE OF A GALAXY'S GLOBULAR CLUSTER POPULATION? [PDF]

open access: yes, 2013
We present a catalog of 422 galaxies with published measurements of their globular cluster (GC) populations. Of these, 248 are E galaxies, 93 are S0 galaxies, and 81 are spirals or irregulars.
W. Harris, G. Harris, M. Alessi
semanticscholar   +1 more source

Keck Imaging of the Globular Cluster Systems in the Early--type Galaxies NGC 1052 and NGC 7332

open access: yes, 2001
The presence of two globular cluster subpopulations in early-type galaxies is now the norm rather than the exception. Here we present two more examples for which the host galaxy appears to have undergone a recent merger.
Brodie, Jean P.   +2 more
core   +1 more source

Compact Binaries in Globular Clusters [PDF]

open access: yesInternational Astronomical Union Colloquium, 2004
AbstractIn dense stellar systems the frequent dynamical interactions between stars play a crucial role in the formation and evolution of compact binaries. We study these processes using a novel approach combining a state-of-the- art binary population synthesis code with a simple treatment of dynamical interactions in dense star cluster cores.
Natalia Ivanova, Frederic A. Rasio
openaire   +3 more sources

RR Lyrae Stars Belonging to the Candidate Globular Cluster Patchick 99

open access: yesThe Astrophysical Journal Letters
Patchick 99 is a candidate globular cluster located in the direction of the Galactic bulge, with a proper motion almost identical to the field and extreme field star contamination. A recent analysis suggests it is a low-luminosity globular cluster with a
Evan Butler   +18 more
doaj   +1 more source

The Extended Baryonic Halo of NGC 3923

open access: yesGalaxies, 2017
Galaxy halos and their globular cluster systems build up over time by the accretion of small satellites. We can learn about this process in detail by observing systems with ongoing accretion events and comparing the data with simulations.
Bryan W. Miller   +9 more
doaj   +1 more source

The Spectacular Tidal Tails of Globular Cluster M3 (NGC 5272)

open access: yesThe Astrophysical Journal, 2023
We provide a detailed analysis of the tidal tails of the globular cluster M3 (NGC 5272). We first discover clear extratidal structures with a slight S shape near the cluster. This inspires us to examine the existence of its long tidal tails. We highlight
Yong Yang   +4 more
doaj   +1 more source

Thermally Pulsing Asymptotic Giant Branch Star Models and Globular Cluster Planetary Nebulae I: The Model

open access: yes, 2011
Thermally pulsing asymptotic giant branch models of globular cluster stars are calculated using a synthetic model with the goal of reproducing the chemical composition, core masses and other observational parameters of the four known globular cluster ...
Alexander   +56 more
core   +1 more source

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