Probing the interior physics of stars through asteroseismology
C Aerts - Reviews of Modern Physics, 2021 - APS
Yearslong time series of high-precision brightness measurements have been assembled for
thousands of stars with telescopes operating in space. Such data have allowed astronomers …
thousands of stars with telescopes operating in space. Such data have allowed astronomers …
A review of the mixing length theory of convection in 1D stellar modeling
M Joyce, J Tayar - Galaxies, 2023 - mdpi.com
We review the application of the one-dimensional Mixing Length Theory (MLT) model of
convection in stellar interiors and low-mass stellar evolution. We summarize the history of …
convection in stellar interiors and low-mass stellar evolution. We summarize the history of …
From dawn till disc: Milky Way's turbulent youth revealed by the APOGEE+Gaia data
V Belokurov, A Kravtsov - Monthly Notices of the Royal …, 2022 - academic.oup.com
We use accurate estimates of aluminium abundance from the APOGEE Data Release 17
and Gaia Early Data Release 3 astrometry to select a highly pure sample of stars with …
and Gaia Early Data Release 3 astrometry to select a highly pure sample of stars with …
The Gaia–Kepler stellar properties catalog. I. Homogeneous fundamental properties for 186,301 Kepler Stars
TA Berger, D Huber, JL Van Saders… - The Astronomical …, 2020 - iopscience.iop.org
An accurate and precise Kepler Stellar Properties Catalog is essential for the interpretation
of the Kepler exoplanet survey results. Previous Kepler Stellar Properties Catalogs have …
of the Kepler exoplanet survey results. Previous Kepler Stellar Properties Catalogs have …
StarHorse results for spectroscopic surveys and Gaia DR3: Chrono-chemical populations in the solar vicinity, the genuine thick disk, and young alpha-rich stars
ABA Queiroz, F Anders, C Chiappini… - Astronomy & …, 2023 - aanda.org
The Gaia mission has provided an invaluable wealth of astrometric data for more than a
billion stars in our Galaxy. The synergy between Gaia astrometry, photometry, and …
billion stars in our Galaxy. The synergy between Gaia astrometry, photometry, and …
The second APOKASC catalog: the empirical approach
MH Pinsonneault, YP Elsworth, J Tayar… - The Astrophysical …, 2018 - iopscience.iop.org
We present a catalog of stellar properties for a large sample of 6676 evolved stars with
Apache Point Observatory Galactic Evolution Experiment spectroscopic parameters and …
Apache Point Observatory Galactic Evolution Experiment spectroscopic parameters and …
Dynamical heating across the Milky Way disc using APOGEE and Gaia
JT Mackereth, J Bovy, HW Leung… - Monthly Notices of …, 2019 - academic.oup.com
The kinematics of the Milky Way disc as a function of age are well measured at the solar
radius, but have not been studied over a wider range of Galactocentric radii. Here, we …
radius, but have not been studied over a wider range of Galactocentric radii. Here, we …
Age dissection of the Milky Way discs: Red giants in the Kepler field
Ensemble studies of red-giant stars with exquisite asteroseismic (Kepler), spectroscopic
(APOGEE), and astrometric (Gaia) constraints offer a novel opportunity to recast and …
(APOGEE), and astrometric (Gaia) constraints offer a novel opportunity to recast and …
Galactic Archaeology with asteroseismic ages: Evidence for delayed gas infall in the formation of the Milky Way disc
Context. Precise stellar ages from asteroseismology have become available and can help to
set stronger constraints on the evolution of the Galactic disc components. Recently …
set stronger constraints on the evolution of the Galactic disc components. Recently …
On the origin of the chemical bimodality of disc stars: a tale of merger and migration
T Buck - Monthly Notices of the Royal Astronomical Society, 2020 - academic.oup.com
ABSTRACT The Milky Way's (MW) stellar disc exhibits a bimodality in the [Fe/H] versus
[α/Fe] plane, showing a distinct high-and low-α sequences whose origin is still under debate …
[α/Fe] plane, showing a distinct high-and low-α sequences whose origin is still under debate …