Results 1 to 10 of about 1,046 (265)
r-process Abundance Patterns in the Globular Cluster M92
Whereas light-element abundance variations are a hallmark of globular clusters, there is little evidence for variations in neutron-capture elements. A significant exception is M15, which shows a star-to-star dispersion in neutron-capture abundances of at
Evan N. Kirby +2 more
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Variable stars in the globular cluster M 13 [PDF]
10 pages, 9 figures, 5 tables, accepted for publication in ...
Kopacki, G. +2 more
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JWST/NIRCam Probes Young Star Clusters in the Reionization Era Sunrise Arc
Star cluster formation in the early universe and its contribution to reionization remains largely unconstrained to date. Here we present JWST/NIRCam imaging of the most highly magnified galaxy known at z ∼ 6, the Sunrise arc.
Eros Vanzella +29 more
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Variable stars in the globular cluster M 92 [PDF]
AbstractResults of a search for variable stars in the central region of the Oosterhoff II type globular cluster M92 are presented.
openaire +2 more sources
A JWST Project on 47 Tucanae: NIRSpec Spectroscopy of Multiple Populations among M Dwarfs
We present the first spectroscopic estimates of the chemical abundance of M dwarf stars in a globular cluster (GC), namely 47 Tucanae. By exploiting NIRSpec on board the James Webb Space Telescope, we gathered low-resolution spectra for 28 stars with ...
A. F. Marino +14 more
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A meta-analysis of seismic ages determined for individual stars in the well-studied open and globular clusters NGC 6819, NGC 6791, M67, M4, M19, M80, and M9 reveals both high variance across measurements and a possible discrepancy with independent ...
Jamie Tayar, Meridith Joyce
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Predictions for Self-Pollution in Globular Cluster Stars [PDF]
Full evolutionary models have been built to follow the phases of asymptotic giant branch evolution with mass loss for metal mass fractions from Z=0.0002 to Z=0.004. For the first time, we find that temperatures close to or even larger than 10^8 K are achieved at low Z; the full CNO cycle operates at the base of the envelope, the Oxygen abundance for ...
Ventura P. 1 +3 more
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Rotation and Hα Emission in a Young SMC Cluster: A Spectroscopic View of NGC 330
We present an analysis of high-resolution optical spectra recorded for 30 stars of the split extended main-sequence turnoff of the young (∼40 Myr) Small Magellanic Cloud globular cluster NGC 330.
Paul I. Cristofari +6 more
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Are there S stars in galactic globular clusters? [PDF]
Deux etoiles geantes rouges dans NGC 6723 montrent des bandes ZrO augmentees. Comparaisons avec les geantes de 47 Tuc et analogie avec les etoiles des Nuages de Magellan.
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The Spatial Distribution of Intracluster Globular Clusters in the Fornax Cluster
We investigate the spatial distribution of the intracluster globular clusters (ICGCs) detected in the core of the Fornax galaxy cluster. By separately modeling different components of the observed population of globular clusters (GCs), we confirm the ...
Raffaele D’Abrusco +8 more
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