Results 1 to 10 of about 1,884 (262)
Solar and stellar photospheric abundances
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 +5 more sources
Accuracy and Precision of Industrial Stellar Abundances [PDF]
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.
Ulrike Heiter, Paula Jofre
exaly +4 more sources
Stellar abundances of beryllium and CUBES [PDF]
11 pages, 8 figures. To appear in Astrophysics and Space Science "Special Issue: UV Astronomy 3", Proceedings of the ESO/NUVA/IAG Workshop on Challenges in UV Astronomy, ESO Garching, 7-11 October ...
R Smiljanic
exaly +3 more sources
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
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
Chemical Analysis of the Brightest Star of the Cetus II Ultrafaint Dwarf Galaxy Candidate
We present a detailed chemical abundance analysis of the brightest star in the ultrafaint dwarf (UFD) galaxy candidate Cetus II from high-resolution Magellan/MIKE spectra.
K. B. Webber +44 more
doaj +1 more source
Theoretical prediction of surface stellar abundances of light elements–lithium, beryllium, and boron–represents one of the most interesting open problems in astrophysics.
E. Tognelli +14 more
doaj +1 more source
Robust Data-driven Metallicities for 175 Million Stars from Gaia XP Spectra
We derive and publish data-driven estimates of stellar metallicity [M/H] for ∼175 million stars with low-resolution XP spectra published in Gaia DR3.
René Andrae +2 more
doaj +1 more source
Clustering in the stellar abundance space [PDF]
15 pages, 13 figures, accepted by MNRAS, author scientific names were ...
Boesso, R., Rocha-Pinto, H. J.
openaire +2 more sources
Chemical abundances of the Typhon stellar stream
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 +2 more sources

