Results 61 to 70 of about 307 (107)
Condensation time of the solar nebula from extinct I in primitive meteorites. [PDF]
Lewis RS, Anders E.
europepmc +1 more source
Neutron capture cross section measurements for nuclear astrophysics at CERN n TOF
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]
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
Recent progress and future prospects of the early solar system chronology. [PDF]
Amelin Y, Yin QZ.
europepmc +1 more source
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]
Hu HM +13 more
europepmc +1 more source
Thorium/neodymium cosmochronology and Galactic chemical evolution
G. J. Mathews, D. N. Schramm
openaire +1 more source
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
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
© 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

