Astrophysics with presolar stardust
DD Clayton, LR Nittler - Annu. Rev. Astron. Astrophys., 2004 - annualreviews.org
▪ Abstract Meteorites and interplanetary dust particles contain presolar stardust grains: solid
samples of stars that can be studied in the laboratory. The stellar origin of the grains is …
samples of stars that can be studied in the laboratory. The stellar origin of the grains is …
Presolar stardust in meteorites: recent advances and scientific frontiers
LR Nittler - Earth and Planetary Science Letters, 2003 - Elsevier
Grains of stardust that formed in stellar outflows prior to the formation of the solar system
survive intact as trace constituents of primitive meteorites. The presolar origin of the grains is …
survive intact as trace constituents of primitive meteorites. The presolar origin of the grains is …
Stellar yields from metal-rich asymptotic giant branch models
We present new theoretical stellar yields and surface abundances for three grids of metal-
rich asymptotic giant branch (AGB) models. Post-processing nucleosynthesis results are …
rich asymptotic giant branch (AGB) models. Post-processing nucleosynthesis results are …
Cool bottom processes on the thermally pulsing asymptotic giant branch and the isotopic composition of circumstellar dust grains
We examine the effects of cool bottom processing (CBP) on the isotopic ratios 18 O/16 O, 17
O/16 O, 14 N/15 N, 26 Al/27 Al, C/O, and N/O in the convective envelope during the …
O/16 O, 14 N/15 N, 26 Al/27 Al, C/O, and N/O in the convective envelope during the …
Short-lived nuclei in the early Solar System: Possible AGB sources
The abundances of short-lived radionuclides in the early Solar System (ESS) are reviewed,
as well as the methodology used in determining them. These results are compared with the …
as well as the methodology used in determining them. These results are compared with the …
Heavy-element yields and abundances of asymptotic giant branch models with a Small Magellanic Cloud metallicity
We present new theoretical stellar yields and surface abundances for asymptotic giant
branch (AGB) models with a metallicity appropriate for stars in the Small Magellanic Cloud …
branch (AGB) models with a metallicity appropriate for stars in the Small Magellanic Cloud …
[BOOK][B] Stellar explosions: hydrodynamics and nucleosynthesis
J Jose - 2016 - books.google.com
Written by a specialist in stellar astrophysics, this book presents a rigorous but accessible
treatment of the physics of stellar explosions from a multidisciplinary perspective at the …
treatment of the physics of stellar explosions from a multidisciplinary perspective at the …
Presolar grains from meteorites: Remnants from the early times of the solar system
This review provides an introduction to presolar grains–preserved stardust from the
interstellar molecular cloud from which our solar system formed–found in primitive …
interstellar molecular cloud from which our solar system formed–found in primitive …
Can extra mixing in RGB and AGB stars be attributed to magnetic mechanisms?
It is known that there must be some weak form of transport (called cool bottom processing, or
CBP) acting in low-mass red giant branch (RGB) and asymptotic giant branch (AGB) stars …
CBP) acting in low-mass red giant branch (RGB) and asymptotic giant branch (AGB) stars …
Production of aluminium and the heavy magnesium isotopes in asymptotic giant branch stars
We investigate the production of aluminium and magnesium in asymptotic giant branch
models covering a wide range in mass and composition. We evolve models from the pre …
models covering a wide range in mass and composition. We evolve models from the pre …