On the metallicity dependence of crystalline silicates in oxygen-rich asymptotic giant branch stars and red supergiants [PDF]
O. C. Jones +12 more
openalex +1 more source
Carbon Stars as Standard Candles: An Empirical Test for the Reddening, Metallicity, and Age Sensitivity of the J-region Asymptotic Giant Branch (JAGB) Method [PDF]
Abigail J. Lee
openalex +1 more source
Phosphorus-bearing molecules PO and PN at the edge of the Galaxy. [PDF]
Koelemay LA, Gold KR, Ziurys LM.
europepmc +1 more source
Evolution and Nucleosynthesis in Extremely Metal-Poor, Asymptotic Giant Branch Stars [PDF]
Nobuyuki Iwamoto
openalex +1 more source
Li Evolution among Stars of Low/Intermediate Mass: the Metal-deficient Open Cluster NGC 2204
We have analyzed high-dispersion spectra in the Li 6708 Å region for 167 stars within the anticenter cluster NGC 2204. From 105 probable members, abundance analysis of 45 evolved stars produces [Fe/H] = −0.40 ± 0.12, [Si/Fe] = 0.14 ± 0.12, [Ca/Fe] = 0.29
Barbara J. Anthony-Twarog +4 more
doaj +1 more source
87th Annual Meeting of the Meteoritical Society 2025: Abstracts
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 30-350, August 2025.
wiley +1 more source
Mixing and Magnetic Fields in Asymptotic Giant Branch Stars in the Framework of FRUITY Models [PDF]
D. Vescovi
openalex +1 more source
The 13C(α, n)16O reaction is considered to be the most important neutron source for the s-process main component in low-mass asymptotic giant branch stars.
Trippella Oscar, La Cognata Marco
doaj +1 more source
Crystallinity versus mass-loss rate in asymptotic giant branch stars [PDF]
F. Kemper +3 more
openalex +1 more source
Discovery of a Metal-poor Red Giant Star with the Highest Ultralithium Enhancement
We present the discovery of 2MASS J05241392−0336543 (hereafter J0524−0336), a very metal-poor ([Fe/H] = −2.43 ± 0.16), highly r -process-enhanced ([Eu/Fe] = +1.34 ± 0.10) Milky Way halo field red giant star, with an ultrahigh Li abundance of A (Li, 3D ...
Jeremy Kowkabany +12 more
doaj +1 more source

