Results 101 to 110 of about 48,373 (195)

From the s-Process to the i-Process: A New Perspective on the Chemical Enrichment of Extrinsic Stars

open access: yesGalaxies
Separating stars enriched in the s- and r-processes of nucleosynthesis is usually achieved by analyzing the element ratios of s-process elements (like Ba or La) to r-process elements (like Eu).
Sophie Van Eck   +11 more
doaj   +1 more source

The heavy-element abundances of AGB stars and the angular momentum conservation model of wind accretion for barium stars [PDF]

open access: yes, 2000
Adpoting new s-process nucleosynthesis scenario and branch s-process path, we calculate the heavy-element abundances and C/O ratio of solar metallicity 3M_sun TP-AGB stars.
Liang, Y. C., Zhang, B., Zhao, G.
core   +1 more source

87th Annual Meeting of the Meteoritical Society 2025: Contents

open access: yes
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 2-29, August 2025.
wiley   +1 more source

87th Annual Meeting of the Meteoritical Society 2025: Abstracts

open access: yes
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 30-350, August 2025.
wiley   +1 more source

Explosive Nucleosynthesis

open access: yes, 2022
Cosmic nucleosynthesis had been one of INTEGRAL’s major science targets. The SPI spectrometer delivered important measurements, both from targets of opportunity in the form of stellar explosions and their shortlived radionuclides, and from cumulative emission of long-lived radioactive isotopes. We review the lessons learned on explosive nucleosynthesis
openaire   +1 more source

Recent Advances in Understanding R-Process Nucleosynthesis in Metal-Poor Stars and Stellar Systems

open access: yesUniverse
The rapid neutron-capture process (r-process) is responsible for the creation of roughly half of the elements heavier than iron, including precious metals like silver, gold, and platinum, as well as radioactive elements such as thorium and uranium ...
Avrajit Bandyopadhyay, Timothy C. Beers
doaj   +1 more source

Nucleosynthesis of Cobalt and Copper

open access: yesGalaxies
Chemical abundances of cobalt (Co; Z = 27) and copper (Cu; Z = 29) in bulge and halo stars are presented and compared with chemical evolution models.
Beatriz Barbuy   +2 more
doaj   +1 more source

Universality and variability of the heavy r-process element abundance pattern from a nonequilibrium approach

open access: yesFrontiers in Astronomy and Space Sciences
A striking feature in the observed chemical composition of the majority of stars is the universality of the relative abundances of the heavy elements, although some outliers exist.
David Blaschke   +6 more
doaj   +1 more source

Home - About - Disclaimer - Privacy