Results 21 to 30 of about 307 (107)

Radioactive nuclei from cosmochronology to habitability

open access: yesProgress in Particle and Nuclear Physics, 2018
Review published in Progress in Particle and Nuclear Physics. The article is being published Open Access, access to the full article is not restricted in any way.
Lugaro, Maria   +2 more
openaire   +4 more sources

The Nuclear Astrophysics Program at the CERN n_TOF Facility: Results and Perspectives

open access: yesUniverse
The CERN n_TOF facility is a research infrastructure specifically designed for studying neutron-induced nuclear reactions. Pulsed white neutron beams are delivered toward three experimental areas, two of them at different baselines to apply the time-of ...
P. M. Milazzo   +2 more
doaj   +1 more source

Thresholds on star formation and the chemical evolution of galactic discs: cosmochronology and the age of the Galaxy [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 1996
Latex version 3.1, 12 pages + 15 figures, MNRAS in press, replaces earlier version in which the postscript figures had become ...
Chamcham, K., Hendry, M. A.
openaire   +2 more sources

In situ single‐spot Rb/Sr cosmochronology of roedderite in the Ribbeck aubrite (asteroid 2024 BX1)

open access: yesMeteoritics &Planetary Science, Volume 61, Issue 5, Page 768-781, May 2026.
Abstract The mineralogy and textures of several fragments from the Ribbeck aubrite were analyzed using a combination of scanning electron microscopy, electron microprobe analysis, μRaman spectroscopy, and laser ablation inductively coupled reaction cell mass spectrometry (LA‐ICP‐MS/MS).
Christopher J. Barnes   +6 more
wiley   +1 more source

White dwarf cosmochronology: Techniques and uncertainties [PDF]

open access: yesProceedings of the International Astronomical Union, 2008
AbstractWhite dwarfs represent the endpoint of the evolution of the large majority of stars formed in the Galaxy. In the last two decades observations and theory have improved to a level that makes possible to employ white dwarfs for determining ages of the stellar populations in the solar neighborhood, and in the nearest star clusters.
openaire   +1 more source

Galactic Chemical Evolution and Nucleocosmochronology: Standard Model with Terminated Infall [PDF]

open access: yes, 1984
Some exactly soluble families of models for the chemical evolution of the Galaxy are presented. The parameters considered include gas mass, the age-metallicity relation, the star mass vs. metallicity, the age distribution, and the mean age of dwarfs.
Clayton, Donald D
core   +1 more source

The Presolar Heritage of 50Ti and 26Al Heterogeneity in the Protoplanetary Disk

open access: yesThe Astrophysical Journal
Nucleosynthetic isotope anomalies have been documented within the solar protoplanetary disk for several isotopes, including ^48 Ca, ^50 Ti, ^54 Cr, ^94 Mo, and ^96 Zr.
Kirsten K. Larsen   +5 more
doaj   +1 more source

Cosmochronology after Allende

open access: yesThe Astrophysical Journal, 1979
Recent data on isotopic anomalies of various elements in meteorites are interpreted in the picture of the birth of the Sun in a stellar OB association. The following points are suggested by this analysis. (a) The standard picture of stellar nucleosynthesis by an exponentially decreasing stellar activity throughout the galactic life remains tenable. (b)
openaire   +1 more source

238U/235U systematics in terrestrial uranium-bearing minerals [PDF]

open access: yes, 2012
The present-day 238U/235U ratio has fundamental implications for uranium-lead geochronology and cosmochronology. A value of 137.88 has previously been considered invariant and has been used without uncertainty to calculate terrestrial mineral ages.
McLean, Noah   +3 more
core   +1 more source

White Dwarfs: Cosmological and Galactic Probes [PDF]

open access: yes, 2005
The emphasis on white dwarf stars and cosmology arises from the most recent advances in cosmological and galactic structure research in which white dwarf stars are playing a very prominent role. Examples are Type Ia supernovae (i.e.
Shipman, Harry L   +2 more
core   +1 more source

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