Results 11 to 20 of about 250,517 (293)

Solar and stellar photospheric abundances [PDF]

open access: yesLiving Reviews in Solar Physics, 2016
The determination of photospheric abundances in late-type stars from spectroscopic observations is a well-established field, built on solid theoretical foundations.
Carlos Allende Prieto   +1 more
exaly   +6 more sources

Chemical abundances of the Typhon stellar stream [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2022
ABSTRACT We present the first high-resolution chemical abundances of seven stars in the recently discovered high-energy stream Typhon. Typhon stars have apocentres r ≳ 100 kpc, making this the first detailed chemical picture of the Milky Way’s very distant stellar halo.
Alexander P Ji   +4 more
openaire   +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.
Suda, Takuma, Takuma Suda
openaire   +4 more sources

Stellar abundances and nucleosynthesis [PDF]

open access: yes, 1974
Stellar abundances are essential parameters for many branches of astronomy. They are also particularly important as tests for theories of nucleosynthesis. Despite the encouraging results from band photometry, detailed spectroscopic analyses are still important in furthering knowledge of physical processes occurring in a variety of stellar objects. This
Ellis, R, Ellis, Richard S.
core   +4 more sources

Stellar Abundances in the Solar Neighborhood [PDF]

open access: yesThe Astronomical Journal, 2012
The only elements that were made in significant quantity during the Big Bang were hydrogen and helium, and to a lesser extent lithium.  Depending on the initial mass of a star, it may eject some or all of the unique, newly formed elements into the interstellar medium.
Hinkel, Natalie R.   +4 more
core   +6 more sources

THE RAVE CATALOG OF STELLAR ELEMENTAL ABUNDANCES: FIRST DATA RELEASE [PDF]

open access: yesThe Astronomical Journal, 2011
We present chemical elemental abundances for $36,561$ stars observed by the RAdial Velocity Experiment (RAVE), an ambitious spectroscopic survey of our Galaxy at Galactic latitudes $|$b$|>25^{\circ}$ and with magnitudes in the range 9$
Zwitter, Tomaž   +23 more
openaire   +7 more sources

Updated opacities from the opacity project [PDF]

open access: yes, 2005
Using the code autostructure, extensive calculations of inner-shell atomic data have been made for the chemical elements He, C, N, O, Ne, Na, Mg, Al, Si, S, Ar, Ca, Cr, Mn, Fe and Ni.
Bautista, M.A.   +7 more
core   +4 more sources

LRPayne: Stellar parameters and abundances from low-resolution spectra

open access: yesAstronomy & Astrophysics
Aims. This paper introduces LRPayne, a novel algorithm designed for the efficient determination of stellar parameters and chemical abundances from low-resolution optical spectra, with a primary focus on data from large-scale galactic surveys such as ...
Vernekar Nagaraj   +6 more
doaj   +2 more sources

On the Hunt for the Origins of the Orphan–Chenab Stream: Detailed Element Abundances with APOGEE and Gaia

open access: yesThe Astrophysical Journal, 2023
Stellar streams in the Galactic halo are useful probes of the assembly of galaxies like the Milky Way. Many tidal stellar streams that have been found in recent years are accompanied by a known progenitor globular cluster or dwarf galaxy.
Keith Hawkins   +10 more
doaj   +1 more source

The Metallicity and Distance of Leo A from Blue Supergiants

open access: yesThe Astrophysical Journal, 2023
We have obtained high-quality spectra of blue supergiant candidates in the dwarf irregular galaxy Leo A with the Low Resolution Imaging Spectrometer at the Keck I telescope.
Miguel A. Urbaneja   +2 more
doaj   +1 more source

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