Results 31 to 40 of about 64,475 (321)

Stellar Parameters and Chemical Abundances Estimated from LAMOST-II DR8 MRS Based on Cycle-StarNet

open access: yesThe Astrophysical Journal Supplement Series, 2023
Deriving stellar atmospheric parameters and chemical abundances from stellar spectra is crucial for understanding the evolution of the Milky Way. By performing a fitting with MARCS model atmospheric theoretical synthetic spectra combined with a domain ...
Rui Wang   +5 more
doaj   +1 more source

Nitrogen Production in Starburst Galaxies Detected by GALEX [PDF]

open access: yes, 2007
We investigate the production of nitrogen in star-forming galaxies with ultraviolet (UV) radiation detected by the Galaxy Evolution Explorer Satellite (GALEX).
Barlow, Tom A.   +24 more
core   +4 more sources

Assessing stellar yields in Galaxy chemical evolution: Observational stellar abundance patterns

open access: yesMonthly Notices of the Royal Astronomical Society, 2023
ABSTRACTOne-zone Galactic chemical evolution (GCE) models have provided useful insights on a great wealth of average abundance patterns in many environments, especially for the Milky Way and its satellites. However, the scatter of such abundance patterns is still a challenging aspect to reproduce.
Jinning Liang, Eda Gjergo, XiLong Fan
openaire   +2 more sources

On the Galactic chemical evolution of sulphur. Sulphur abundances from the [S i] 1082 nm line in giants [PDF]

open access: yes, 2013
Context. The Galactic chemical evolution of sulphur is still under debate. At low metallicities some studies find no correlation between [S/Fe] and [Fe/H], others find [S/Fe] increasing towards lower metallicities, and still others find a combination of ...
Dupree, A. K., Matrozis, E., Ryde, N.
core   +1 more source

Accuracy and Precision of Industrial Stellar Abundances [PDF]

open access: yesAnnual Review of Astronomy and Astrophysics, 2019
There has been an incredibly large investment in obtaining high-resolution stellar spectra for determining chemical abundances of stars. This information is crucial to answer fundamental questions in astronomy by constraining the formation and evolution scenarios of the Milky Way as well as the stars and planets residing in it. We have just entered a
Jofré, Paula   +2 more
openaire   +3 more sources

Forming super-Mercuries: Role of stellar abundances

open access: yesAstronomy & Astrophysics, 2023
Rocky exoplanets with bulk iron mass fraction of more than 60%, known as super-Mercuries, appear to be preferentially hosted by stars with higher iron mass fraction than that of the Sun. It is unclear whether these iron-rich planets can form in the disc or whether giant impacts are necessary for their formation.
Jingyi Mah, Bertram Bitsch
openaire   +2 more sources

Beryllium abundances along the evolutionary sequence of the open cluster IC 4651 - New test for hydrodynamical stellar models

open access: yes, 2009
[abridged] Previous analyses of lithium abundances in main sequence and red giant stars have revealed the action of mixing mechanisms other than convection in stellar interiors.
C. Charbonnel   +8 more
core   +2 more sources

Elemental Abundances in M31: Alpha and Iron Element Abundances from Low-Resolution Resolved Stellar Spectroscopy in the Stellar Halo [PDF]

open access: yes, 2019
Measurements of [Fe/H] and [$\alpha$/Fe] can probe the minor merging history of a galaxy, providing a direct way to test the hierarchical assembly paradigm.
Cunningham, Emily C.   +4 more
core   +3 more sources

SAGA: Stellar Abundances for Galatic Archeology [PDF]

open access: yesProceedings of XII International Symposium on Nuclei in the Cosmos — PoS(NIC XII), 2013
A tutorial for the Stellar Abundances for Galactic Archaeology (SAGA) database is presented. This paper describes the outline of the database, reports the current status of the data compilation and known problems, and presents plans for future updates and extensions.
openaire   +2 more sources

Validating Stellar Abundance Measurements from Multiresolution Spectroscopy

open access: yesThe Astrophysical Journal Supplement Series, 2023
Abstract Large-scale surveys will provide spectroscopy for ∼50 million resolved stars in the Milky Way and Local Group. However, these data will have a high degree of heterogeneity and most will be low-resolution (R < 10,000), posing challenges to measuring consistent and reliable stellar labels.
Nathan R. Sandford   +2 more
openaire   +3 more sources

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