Results 21 to 30 of about 992,258 (306)

How accretion of planet-forming disks influences stellar abundances [PDF]

open access: yesAstronomy & Astrophysics, 2023
Millimeter sized dust grains experience radial velocities exceeding the gas velocities by orders of magnitude. The viscous evolution of the accretion disk adds disk material onto the central star's convective envelope, influencing its elemental ...
Le'on-Alexander Huhn, B. Bitsch
semanticscholar   +1 more source

The SAPP pipeline for the determination of stellar abundances and atmospheric parameters of stars in the core program of the PLATO mission [PDF]

open access: yesAstronomy & Astrophysics, 2021
We introduce the SAPP (Stellar Abundances and atmospheric Parameters Pipeline), the prototype of the code that will be used to determine parameters of stars observed within the core program of the PLATO space mission.
M. Gent   +27 more
semanticscholar   +1 more source

Residual Abundances in GALAH DR3: Implications for Nucleosynthesis and Identification of Unique Stellar Populations [PDF]

open access: yesAstrophysical Journal, 2021
We investigate the [X/Mg] abundances of 16 elements for 82,910 Galactic disk stars from GALAH+ DR3. We fit the median trends of low-Ia and high-Ia populations with a two-process model, which describes stellar abundances in terms of a prompt core-collapse
E. Griffith   +5 more
semanticscholar   +1 more source

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

The Sixth Data Release of the Radial Velocity Experiment (Rave). II. Stellar Atmospheric Parameters, Chemical Abundances, and Distances [PDF]

open access: yesAstronomical Journal, 2020
We present part 2 of the sixth and final Data Release (DR6) of the Radial Velocity Experiment (Rave), a magnitude-limited ( ) spectroscopic survey of Galactic stars randomly selected in Earth’s southern hemisphere. The Rave medium-resolution spectra (R ∼
M. Steinmetz   +61 more
semanticscholar   +1 more source

Clustering in the stellar abundance space [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2017
15 pages, 13 figures, accepted by MNRAS, author scientific names were ...
Boesso, R., Rocha-Pinto, H. J.
openaire   +2 more sources

The Southern Stellar Stream Spectroscopic Survey (S5): Chemical Abundances of Seven Stellar Streams [PDF]

open access: yesAstronomical Journal, 2020
We present high-resolution Magellan/MIKE spectroscopy of 42 red giant stars in seven stellar streams confirmed by the Southern Stellar Stream Spectroscopic Survey (S5): ATLAS, Aliqa Uma, Chenab, Elqui, Indus, Jhelum, and Phoenix.
A. Ji   +18 more
semanticscholar   +1 more source

Chemical Analysis of the Brightest Star of the Cetus II Ultrafaint Dwarf Galaxy Candidate

open access: yesThe Astrophysical Journal, 2023
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

Stellar Tidal Disruption Events with Abundances and Realistic Structures (STARS): Library of Fallback Rates [PDF]

open access: yesAstrophysical Journal, 2020
We present the STARS library, a grid of tidal disruption event (TDE) simulations interpolated to provide the mass fallback rate (dM/dt) to the black hole for a main-sequence star of any stellar mass, stellar age, and impact parameter.
J. Law-Smith   +4 more
semanticscholar   +1 more source

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