Results 81 to 90 of about 21,814 (256)
To appear in the proceedings of the May 2003 STScI Symposium, ``The Local Group as an Astrophysical Laboratory''; 17 pages, 11 figures.
openaire +2 more sources
Extremely Metal-Poor Asymptotic Giant Branch Stars
Little is known about the first stars, but hints on this stellar population can be derived from the peculiar chemical composition of the most metal-poor objects in the Milky Way and in resolved stellar populations of nearby galaxies.
Mario Cirillo +2 more
doaj +1 more source
Key Points A method is described to obtain high precision Sn isotope ratios using the double spike technique in geological reference materials containing 0.03 to 7 μg g−1 of Sn. δ122/118Sn values are reported for sixteen geological RMs. Improved precision was achieved compared with previous studies by using low concentration Sn analyte.
Dipankar Pathak, Klaus Mezger
wiley +1 more source
Nucleosynthesis in Novae [PDF]
Peer ...
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r-process Nucleosynthesis from Three-dimensional Magnetorotational Core-collapse Supernovae [PDF]
We investigate r-process nucleosynthesis in 3D general-relativistic magnetohydrodynamic simulations of rapidly rotating strongly magnetized core collapse.
P. Mösta +6 more
semanticscholar +1 more source
Mixing and Magnetic Fields in Asymptotic Giant Branch Stars in the Framework of FRUITY Models
In the last few years, the modeling of asymptotic giant branch (AGB) stars has been much investigated, both focusing on nucleosynthesis and stellar evolution aspects. Recent advances in the input physics required for stellar computations made it possible
Diego Vescovi
doaj +1 more source
Key Points Isotopic reference materials are rarely cross‐examined. An optimised regression model and MC‐ICP‐MS offer a cost‐effective way to assess the reliability of values assigned to multi‐isotope reference materials. A significant lack of consistency has been observed in the long‐standing isotopic reference materials for nickel and zinc. Calibrated
Juris Meija +4 more
wiley +1 more source
PRIMORDIAL NUCLEOSYNTHESIS REDUX
The abundances of D, He-3, He-4, and Li-7, are presently recalculated within the framework of primordial nucleosynthesis in the standard hot big band model, in order to estimate the primordial abundances of the light elements. A comparison between theory and experiment demonstrates the consistency of standard model predictions; the baryon density ...
Terry P. Walker +4 more
openaire +1 more source
Neutrinos and nucleosynthesis of elements [PDF]
T. Fischer +5 more
semanticscholar +1 more source
Signatures of hypermassive neutron star lifetimes on r-process nucleosynthesis in the disc ejecta from neutron star mergers [PDF]
We investigate the nucleosynthesis of heavy elements in the winds ejected by accretion discs formed in neutron star mergers. We compute the element formation in disc outflows from hypermassive neutron star (HMNS) remnants of variable lifetime, including ...
J. Lippuner +6 more
semanticscholar +1 more source

