Results 61 to 70 of about 307 (107)

Neutron capture cross section measurements for nuclear astrophysics at CERN n TOF

open access: yes
A series of neutron capture cross section measurements of interest to nuclear astrophysics have been recently performed at n TOF, the neutron spallation source operating at CERN.
Pretel Sánchez, Carme   +3 more
core  

Understanding the Cool DA White Dwarf Pulsator, G29–38 [PDF]

open access: yes, 1997
The white dwarfs are promising laboratories for the study of cosmochronology and stellar evolution. Through observations of the pulsating white dwarfs, we can measure their internal structures and compositions, critical to understanding post main ...
Nitta, A.   +36 more
core  

Sub-epsilon natural <sup>234</sup>U/<sup>238</sup>U measurements refine the <sup>234</sup>U half-life and U-Th geochronology. [PDF]

open access: yesSci Adv
Hu HM   +13 more
europepmc   +1 more source

Thorium/neodymium cosmochronology and Galactic chemical evolution

open access: yesThe Astrophysical Journal, 1988
G. J. Mathews, D. N. Schramm
openaire   +1 more source

The effect of 22Ne diffusion in the evolution and pulsational properties of white dwarfs with solar metallicity progenitors

open access: yes, 2019
Because of the large neutron excess of 22Ne, sedimentation of this isotope occurs rapidly in the interior of white dwarfs. This process releases an additional amount of energy, thus delaying the cooling times of the white dwarf.
Isern, J.   +7 more
core  

New cooling sequences for old white dwarfs

open access: yes
We present full evolutionary calculations appropriate for the study of hydrogen-rich DA white dwarfs. This is done by evolving white dwarf progenitors from the zero-age main sequence, through the core hydrogen-burning phase, the helium-burning phase, and
Miller Bertolami, Marcelo M   +6 more
core  

The effect of 22Ne diffusion in the evolution and pulsational properties of white dwarfs with solar metallicity prgenitors

open access: yes
© 2016. The American Astronomical Society. All rights reserved. Because of the large neutron excess of 22Ne, sedimentation of this isotope occurs rapidly in the interior of white dwarfs. This process releases an additional amount of energy, thus delaying
Miller Bertolami, Marcelo M   +7 more
core  

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