Results 101 to 110 of about 22,085 (227)

On the metallicity dependence of crystalline silicates in oxygen-rich asymptotic giant branch stars and red supergiants [PDF]

open access: bronze, 2012
O. C. Jones   +12 more
openalex   +1 more source

Li Evolution among Stars of Low/Intermediate Mass: the Metal-deficient Open Cluster NGC 2204

open access: yesThe Astronomical Journal
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

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

Determining the 13C(α, n)16O absolute cross section through the concurrent application of ANC and THM and astrophysical consequences for the s-process in AGB-LMSs.

open access: yesEPJ Web of Conferences, 2017
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]

open access: bronze, 2001
F. Kemper   +3 more
openalex   +1 more source

Discovery of a Metal-poor Red Giant Star with the Highest Ultralithium Enhancement

open access: yesThe Astrophysical Journal
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

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