Astrophysical Journal, ISSN 0004-637X, 02/2014, Volume 782, Issue 1, pp. 1 - 17
For the very best and brightest asteroseismic solar-type targets observed by Kepler, the frequency precision is sufficient to determine the acoustic depths of...
stars: interiors | stars: oscillations | MODE FREQUENCIES | HELIUM ABUNDANCE | LOW-MASS STARS | MAIN-SEQUENCE | P-MODES | ASTEROSEISMIC ANALYSIS | STELLAR EVOLUTION CODE | ASTRONOMY & ASTROPHYSICS | CONVECTION ZONE | LARGE SEPARATIONS | PHASE-SHIFT | Glitches | Spherical harmonics | Ionization | Stars | Oscillations | Acoustics | Helium | Deviation | Physics - Solar and Stellar Astrophysics | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | CONVECTION | OSCILLATION MODES | STARS | OSCILLATIONS | ACCURACY | SPHERICAL CONFIGURATION | SURFACES
stars: interiors | stars: oscillations | MODE FREQUENCIES | HELIUM ABUNDANCE | LOW-MASS STARS | MAIN-SEQUENCE | P-MODES | ASTEROSEISMIC ANALYSIS | STELLAR EVOLUTION CODE | ASTRONOMY & ASTROPHYSICS | CONVECTION ZONE | LARGE SEPARATIONS | PHASE-SHIFT | Glitches | Spherical harmonics | Ionization | Stars | Oscillations | Acoustics | Helium | Deviation | Physics - Solar and Stellar Astrophysics | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | CONVECTION | OSCILLATION MODES | STARS | OSCILLATIONS | ACCURACY | SPHERICAL CONFIGURATION | SURFACES
Journal Article
Astrophysical Journal, ISSN 0004-637X, 03/2017, Volume 837, Issue 1
Acoustic glitches are regions inside a star where the sound speed or its derivatives change abruptly. These leave a small characteristic oscillatory signature...
stars: fundamental parameters | stars: oscillations | stars: solar-type | stars: interiors | STELLAR OSCILLATION FREQUENCIES | GALACTIC ARCHAEOLOGY | MAIN-SEQUENCE STARS | OPACITY PROJECT | ACOUSTIC GLITCHES | S-FACTOR | ASTROPHYSICS MESA | EXOPLANET HOST STARS | ASTEROSEISMIC DATA | ASTRONOMY & ASTROPHYSICS | SOLAR-TYPE STARS | ACOUSTICS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | CONVECTION | SOUND WAVES | STARS | AMPLITUDES | OSCILLATIONS | IONIZATION | HELIUM | ABUNDANCE | LAYERS
stars: fundamental parameters | stars: oscillations | stars: solar-type | stars: interiors | STELLAR OSCILLATION FREQUENCIES | GALACTIC ARCHAEOLOGY | MAIN-SEQUENCE STARS | OPACITY PROJECT | ACOUSTIC GLITCHES | S-FACTOR | ASTROPHYSICS MESA | EXOPLANET HOST STARS | ASTEROSEISMIC DATA | ASTRONOMY & ASTROPHYSICS | SOLAR-TYPE STARS | ACOUSTICS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | CONVECTION | SOUND WAVES | STARS | AMPLITUDES | OSCILLATIONS | IONIZATION | HELIUM | ABUNDANCE | LAYERS
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 12/2015, Volume 454, Issue 2, pp. 1792 - 1797
We use 4 yr of Kepler photometry to study the non-eclipsing spectroscopic binary KIC 10080943. We find both components to be gamma Doradus/delta Scuti hybrids,...
ORDER G-MODES | FREQUENCIES | PERIOD SPACINGS | SPB | stars: variables: general | TO-CORE ROTATION | stars: individual: KIC 10080943 | MAIN-SEQUENCE | KEPLER | asteroseismology | stars: oscillations | ASTEROSEISMIC MEASUREMENT | PHOTOMETRY | ASTRONOMY & ASTROPHYSICS | binaries: spectroscopic | PULSATIONS | stars: variables: delta Scuti
ORDER G-MODES | FREQUENCIES | PERIOD SPACINGS | SPB | stars: variables: general | TO-CORE ROTATION | stars: individual: KIC 10080943 | MAIN-SEQUENCE | KEPLER | asteroseismology | stars: oscillations | ASTEROSEISMIC MEASUREMENT | PHOTOMETRY | ASTRONOMY & ASTROPHYSICS | binaries: spectroscopic | PULSATIONS | stars: variables: delta Scuti
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 09/2016, Volume 593, p. A120
Context. Gamma Doradus stars (hereafter gamma Dor stars) are known to exhibit gravity- and/or gravito-intertial modes that probe the inner stellar region near...
Methods: data analysis | Stars: fundamental parameters | Asteroseismology | Stars: oscillations | Stars: variables: general | ORDER G-MODES | methods: data analysis | stars: variables: general | TO-CORE ROTATION | ANGULAR-DEPENDENCE | INTERNAL-ROTATION | DELTA-SCUTI | MAIN-SEQUENCE | CORIOLIS-FORCE | STELLAR ASTROPHYSICS MESA | asteroseismology | stars: oscillations | ASTEROSEISMIC MEASUREMENT | ASTRONOMY & ASTROPHYSICS | stars: fundamental parameters | OSCILLATIONS | Coriolis force | Asymptotic properties | Stars | Stellar rotation | Modelling | Boundaries | Signatures | Pulsation | Physics - Solar and Stellar Astrophysics
Methods: data analysis | Stars: fundamental parameters | Asteroseismology | Stars: oscillations | Stars: variables: general | ORDER G-MODES | methods: data analysis | stars: variables: general | TO-CORE ROTATION | ANGULAR-DEPENDENCE | INTERNAL-ROTATION | DELTA-SCUTI | MAIN-SEQUENCE | CORIOLIS-FORCE | STELLAR ASTROPHYSICS MESA | asteroseismology | stars: oscillations | ASTEROSEISMIC MEASUREMENT | ASTRONOMY & ASTROPHYSICS | stars: fundamental parameters | OSCILLATIONS | Coriolis force | Asymptotic properties | Stars | Stellar rotation | Modelling | Boundaries | Signatures | Pulsation | Physics - Solar and Stellar Astrophysics
Journal Article
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, ISSN 0067-0049, 09/2019, Volume 244, Issue 1, p. 18
We present the first data release of the Kepler Smear Campaign, using collateral "smear" data obtained in the Kepler four-year mission to reconstruct light...
PERIOD SPACINGS | stars: variables: general | techniques: photometric | TO-CORE ROTATION | INTERNAL-ROTATION | MAIN-SEQUENCE | SOLAR-TYPE | PULSATING STARS | PHASE MODULATION | stars: early-type | asteroseismology | ASTEROSEISMIC MEASUREMENT | FINDING BINARIES | ASTRONOMY & ASTROPHYSICS | RADIAL-VELOCITIES | stars: rotation
PERIOD SPACINGS | stars: variables: general | techniques: photometric | TO-CORE ROTATION | INTERNAL-ROTATION | MAIN-SEQUENCE | SOLAR-TYPE | PULSATING STARS | PHASE MODULATION | stars: early-type | asteroseismology | ASTEROSEISMIC MEASUREMENT | FINDING BINARIES | ASTRONOMY & ASTROPHYSICS | RADIAL-VELOCITIES | stars: rotation
Journal Article
Astrophysical Journal Supplement Series, ISSN 0067-0049, 2015, Volume 218, Issue 2, pp. 1 - 32
Gamma Doradus stars (hereafter gamma Dor stars) are gravity-mode pulsators of spectral type A or F. Such modes probe the deep stellar interior, offering a...
stars: fundamental parameters | asteroseismology | stars: oscillations | stars: variables: general | ORDER G-MODES | MERCATOR TELESCOPE | TO-CORE ROTATION | SEMICONVECTION | MAIN-SEQUENCE | SPECTRUM ANALYSIS | DELTA SCT | ASTEROSEISMIC MEASUREMENT | ASTRONOMY & ASTROPHYSICS | FREQUENCY G-MODES | PULSATIONS | Spectroscopy | Binary stars | Stars | Binary systems | Spectra | Diagnostic systems | Photometry | Pulsation
stars: fundamental parameters | asteroseismology | stars: oscillations | stars: variables: general | ORDER G-MODES | MERCATOR TELESCOPE | TO-CORE ROTATION | SEMICONVECTION | MAIN-SEQUENCE | SPECTRUM ANALYSIS | DELTA SCT | ASTEROSEISMIC MEASUREMENT | ASTRONOMY & ASTROPHYSICS | FREQUENCY G-MODES | PULSATIONS | Spectroscopy | Binary stars | Stars | Binary systems | Spectra | Diagnostic systems | Photometry | Pulsation
Journal Article
ASTRONOMY & ASTROPHYSICS, ISSN 1432-0746, 07/2017, Volume 603
Context. Stellar rotation affects the transport of chemical elements and angular momentum and is therefore a key process during stellar evolution, which is...
ORDER G-MODES | stars: interiors | B-TYPE STARS | RED GIANTS | TO-CORE ROTATION | INTERNAL-ROTATION | MAIN-SEQUENCE | STELLAR ASTROPHYSICS MESA | EJECTION IMAGER SMEI | asteroseismology | stars: oscillations | ASTEROSEISMIC MEASUREMENT | ASTRONOMY & ASTROPHYSICS | stars: individual: HD201433 | SPACE-BASED PHOTOMETRY | binaries: general | stars: rotation
ORDER G-MODES | stars: interiors | B-TYPE STARS | RED GIANTS | TO-CORE ROTATION | INTERNAL-ROTATION | MAIN-SEQUENCE | STELLAR ASTROPHYSICS MESA | EJECTION IMAGER SMEI | asteroseismology | stars: oscillations | ASTEROSEISMIC MEASUREMENT | ASTRONOMY & ASTROPHYSICS | stars: individual: HD201433 | SPACE-BASED PHOTOMETRY | binaries: general | stars: rotation
Journal Article
ASTRONOMY & ASTROPHYSICS, ISSN 1432-0746, 06/2019, Volume 627
The effects of rotation on stellar evolution are particularly important at low metallicity, when mass loss by stellar winds diminishes and the surface...
stars: evolution | POPULATION SYNTHESIS | TO-CORE ROTATION | MASS-LOSS RATES | DWARF GALAXIES | MAIN-SEQUENCE | ABUNDANCES | stars: abundances | ASTEROSEISMIC MEASUREMENT | EVOLUTION | STAR | COMPACT GALAXIES | ASTRONOMY & ASTROPHYSICS | stars: mass-loss | stars: massive | stars: fundamental parameters | stars: rotation
stars: evolution | POPULATION SYNTHESIS | TO-CORE ROTATION | MASS-LOSS RATES | DWARF GALAXIES | MAIN-SEQUENCE | ABUNDANCES | stars: abundances | ASTEROSEISMIC MEASUREMENT | EVOLUTION | STAR | COMPACT GALAXIES | ASTRONOMY & ASTROPHYSICS | stars: mass-loss | stars: massive | stars: fundamental parameters | stars: rotation
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 05/2019, Volume 485, Issue 3, pp. 3661 - 3680
The angular momentum (AM) evolution of stellar interiors, along with the resulting rotation rates of stellar remnants, remains poorly understood. Asteroseismic...
ANGULAR-MOMENTUM TRANSPORT | stars: interiors | MAGNETIC-FIELDS | stars: evolution | STABILITY | MHD | NEUTRON-STARS | MAIN-SEQUENCE | DYNAMO ACTION | instabilities | DIFFERENTIAL ROTATION | asteroseismology | ASTEROSEISMIC MEASUREMENT | EVOLUTION | ASTRONOMY & ASTROPHYSICS | TURBULENCE | stars: rotation | Physics - Solar and Stellar Astrophysics
ANGULAR-MOMENTUM TRANSPORT | stars: interiors | MAGNETIC-FIELDS | stars: evolution | STABILITY | MHD | NEUTRON-STARS | MAIN-SEQUENCE | DYNAMO ACTION | instabilities | DIFFERENTIAL ROTATION | asteroseismology | ASTEROSEISMIC MEASUREMENT | EVOLUTION | ASTRONOMY & ASTROPHYSICS | TURBULENCE | stars: rotation | Physics - Solar and Stellar Astrophysics
Journal Article
Astrophysical Journal, ISSN 0004-637X, 02/2019, Volume 871, Issue 2, p. 135
The 2D internal rotation of KIC 11145123 has been inferred via asteroseismology. Based on the optimally localized averaging method and a simple three-zone...
stars: Variables: Delta Scuti | stars: Individual (KIC 11145123) | stars: Interiors | stars: Oscillations | stars: Rotation | stars: interiors | CONVECTION | TO-CORE ROTATION | MAIN-SEQUENCE | INVERSION | DIFFERENTIAL ROTATION | stars: oscillations | ASTEROSEISMIC MEASUREMENT | A-TYPE STARS | ASTRONOMY & ASTROPHYSICS | SIMULATIONS | stars: rotation | stars: variables: delta Scuti | stars: individual (KIC 11145123)
stars: Variables: Delta Scuti | stars: Individual (KIC 11145123) | stars: Interiors | stars: Oscillations | stars: Rotation | stars: interiors | CONVECTION | TO-CORE ROTATION | MAIN-SEQUENCE | INVERSION | DIFFERENTIAL ROTATION | stars: oscillations | ASTEROSEISMIC MEASUREMENT | A-TYPE STARS | ASTRONOMY & ASTROPHYSICS | SIMULATIONS | stars: rotation | stars: variables: delta Scuti | stars: individual (KIC 11145123)
Journal Article
Astrophysical Journal, ISSN 0004-637X, 09/2015, Volume 810, Issue 1, pp. 16 - 26
The internal angular momentum distribution of a star is the key to determining its evolution. Fortunately, stellar internal rotation can be probed through...
asteroseismology | stars: oscillations | stars: rotation | stars: individual (KIC 10526294) | SEISMIC EVIDENCE | MASSIVE STARS | ANGULAR-MOMENTUM TRANSPORT | RED GIANTS | TO-CORE ROTATION | MAIN-SEQUENCE | KEPLER | STELLAR ASTROPHYSICS MESA | ASTEROSEISMIC MEASUREMENT | ASTRONOMY & ASTROPHYSICS | CONSTRAINTS | Kernels | Envelopes | Differential rotation | Gravitation | Dipoles | Stars | Rotational | Massive stars | ROTATION | SPACE | ANGULAR MOMENTUM | DIPOLES | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | STAR EVOLUTION | GRAVITATION | OSCILLATION MODES | STARS | OSCILLATIONS | PROBES
asteroseismology | stars: oscillations | stars: rotation | stars: individual (KIC 10526294) | SEISMIC EVIDENCE | MASSIVE STARS | ANGULAR-MOMENTUM TRANSPORT | RED GIANTS | TO-CORE ROTATION | MAIN-SEQUENCE | KEPLER | STELLAR ASTROPHYSICS MESA | ASTEROSEISMIC MEASUREMENT | ASTRONOMY & ASTROPHYSICS | CONSTRAINTS | Kernels | Envelopes | Differential rotation | Gravitation | Dipoles | Stars | Rotational | Massive stars | ROTATION | SPACE | ANGULAR MOMENTUM | DIPOLES | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | STAR EVOLUTION | GRAVITATION | OSCILLATION MODES | STARS | OSCILLATIONS | PROBES
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2015, Volume 450, Issue 3, pp. 3015 - 3029
There are many Slowly Pulsating B (SPB) stars and gamma Dor stars in the Kepler mission data set. The light curves of these pulsating stars have been...
Stars: interiors | Stars: emission-line, be | Asteroseismology | Stars: oscillations | asteroseismology | stars: oscillations | ASTEROSEISMIC MEASUREMENT | stars: interiors | ASTRONOMY & ASTROPHYSICS | TO-CORE ROTATION | DORADUS STARS | FIELD-OF-VIEW | stars: emission-line | DELTA-SCUTI STARS | MAIN-SEQUENCE | KEPLER | Physics - Solar and Stellar Astrophysics
Stars: interiors | Stars: emission-line, be | Asteroseismology | Stars: oscillations | asteroseismology | stars: oscillations | ASTEROSEISMIC MEASUREMENT | stars: interiors | ASTRONOMY & ASTROPHYSICS | TO-CORE ROTATION | DORADUS STARS | FIELD-OF-VIEW | stars: emission-line | DELTA-SCUTI STARS | MAIN-SEQUENCE | KEPLER | Physics - Solar and Stellar Astrophysics
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 05/2018, Volume 476, Issue 3, pp. 3169 - 3184
The delta Sct stars are a diverse group of intermediate-mass pulsating stars located on and near the main sequence within the classical instability strip in...
techniques: photometric | TO-CORE ROTATION | INTERNAL-ROTATION | MAIN-SEQUENCE | SPECTRUM ANALYSIS | SCUTI STARS | PULSATIONAL INSTABILITY | asteroseismology | stars: oscillations | ASTEROSEISMIC MEASUREMENT | COMBINATION FREQUENCIES | ASTRONOMY & ASTROPHYSICS | AMPLITUDE-MODULATION | SPECTROSCOPIC SURVEY | stars: variables: delta Scuti
techniques: photometric | TO-CORE ROTATION | INTERNAL-ROTATION | MAIN-SEQUENCE | SPECTRUM ANALYSIS | SCUTI STARS | PULSATIONAL INSTABILITY | asteroseismology | stars: oscillations | ASTEROSEISMIC MEASUREMENT | COMBINATION FREQUENCIES | ASTRONOMY & ASTROPHYSICS | AMPLITUDE-MODULATION | SPECTROSCOPIC SURVEY | stars: variables: delta Scuti
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 10/2018, Volume 618, p. A24
Context. While rotation has a major impact on stellar structure and evolution, its effects are not well understood. Thanks to high-quality and long-time base...
Methods: data analysis | Stars: fundamental parameters | Asteroseismology | Stars: oscillations | Stars: rotation | Stars: variables: general | ORDER G-MODES | methods: data analysis | ANGULAR-MOMENTUM TRANSPORT | stars: variables: general | NONRADIAL OSCILLATIONS | UNIFORM INTERNAL-ROTATION | TO-CORE ROTATION | PULSATING B-STARS | asteroseismology | stars: oscillations | GAMMA DORADUS STARS | ASTEROSEISMIC MEASUREMENT | STELLAR EVOLUTION | ASTRONOMY & ASTROPHYSICS | 2-DIMENSIONAL MODELS | stars: fundamental parameters | stars: rotation | Physics - Solar and Stellar Astrophysics | Physics | Astrophysics
Methods: data analysis | Stars: fundamental parameters | Asteroseismology | Stars: oscillations | Stars: rotation | Stars: variables: general | ORDER G-MODES | methods: data analysis | ANGULAR-MOMENTUM TRANSPORT | stars: variables: general | NONRADIAL OSCILLATIONS | UNIFORM INTERNAL-ROTATION | TO-CORE ROTATION | PULSATING B-STARS | asteroseismology | stars: oscillations | GAMMA DORADUS STARS | ASTEROSEISMIC MEASUREMENT | STELLAR EVOLUTION | ASTRONOMY & ASTROPHYSICS | 2-DIMENSIONAL MODELS | stars: fundamental parameters | stars: rotation | Physics - Solar and Stellar Astrophysics | Physics | Astrophysics
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2015, Volume 450, Issue 3, pp. 2764 - 2783
The Kepler space mission provided near-continuous and high-precision photometry of about 207 000 stars, which can be used for asteroseismology. However, for...
Stars: abundances | Stars: general | Stars: chemically peculiar | Stars: rotation | GAMMA-DORADUS | stars: general | TO-CORE ROTATION | DELTA-SCUTI STARS | LTE LINE FORMATION | MAIN-SEQUENCE | stars: abundances | ASTEROSEISMIC MEASUREMENT | A-TYPE STARS | ASTRONOMY & ASTROPHYSICS | CHEMICAL-COMPOSITION | stars: chemically peculiar | FUNDAMENTAL PARAMETERS | stars: rotation | OPEN CLUSTER | Physics - Solar and Stellar Astrophysics
Stars: abundances | Stars: general | Stars: chemically peculiar | Stars: rotation | GAMMA-DORADUS | stars: general | TO-CORE ROTATION | DELTA-SCUTI STARS | LTE LINE FORMATION | MAIN-SEQUENCE | stars: abundances | ASTEROSEISMIC MEASUREMENT | A-TYPE STARS | ASTRONOMY & ASTROPHYSICS | CHEMICAL-COMPOSITION | stars: chemically peculiar | FUNDAMENTAL PARAMETERS | stars: rotation | OPEN CLUSTER | Physics - Solar and Stellar Astrophysics
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 07/2017, Volume 469, Issue 1, pp. L118 - L122
We present the analysis of 29.77 d of K2 space photometry of the well-detached massive 4.6 d O+B binary HD 165246 (V = 7.6) obtained during Campaign 9b. This...
binaries: eclipsing | techniques: photometric | stars: variables: general | TO-CORE ROTATION | INTERNAL-ROTATION | KEPLER-MISSION | HEARTBEAT | asteroseismology | ASTEROSEISMIC MEASUREMENT | STAR | ASTRONOMY & ASTROPHYSICS | stars: massive | stars: individual: HD 165246
binaries: eclipsing | techniques: photometric | stars: variables: general | TO-CORE ROTATION | INTERNAL-ROTATION | KEPLER-MISSION | HEARTBEAT | asteroseismology | ASTEROSEISMIC MEASUREMENT | STAR | ASTRONOMY & ASTROPHYSICS | stars: massive | stars: individual: HD 165246
Journal Article
Astrophysical Journal Letters, ISSN 2041-8205, 09/2017, Volume 847, Issue 1, p. L7
A major uncertainty in the theory of stellar evolution is the angular momentum distribution inside stars and its change during stellar life. We compose a...
waves | stars: massive | asteroseismology | stars: oscillations | stars: evolution | stars: rotation | ORDER G-MODES | GAMMA DORADUS STARS | ASTEROSEISMIC MEASUREMENT | ASTRONOMY & ASTROPHYSICS | INTERNAL-ROTATION | MAIN-SEQUENCE | Physics - Solar and Stellar Astrophysics
waves | stars: massive | asteroseismology | stars: oscillations | stars: evolution | stars: rotation | ORDER G-MODES | GAMMA DORADUS STARS | ASTEROSEISMIC MEASUREMENT | ASTRONOMY & ASTROPHYSICS | INTERNAL-ROTATION | MAIN-SEQUENCE | Physics - Solar and Stellar Astrophysics
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 03/2016, Volume 458, Issue 3, pp. 2307 - 2322
We present a spectroscopic survey of known and candidate gamma Doradus stars. The high-resolution, high signal-to-noise spectra of 52 objects were collected by...
Stars: Rotation | Stars: Chemically peculiar | Stars: Abundances | Stars: General | ORDER G-MODES | stars: general | F-TYPE STARS | TO-CORE ROTATION | DELTA-SCUTI STARS | MAIN-SEQUENCE | stars: abundances | STELLAR ASTROPHYSICS MESA | ASTEROSEISMIC MEASUREMENT | EFFECTIVE TEMPERATURE | A-TYPE STARS | ASTRONOMY & ASTROPHYSICS | stars: chemically peculiar | FUNDAMENTAL PARAMETERS | stars: rotation
Stars: Rotation | Stars: Chemically peculiar | Stars: Abundances | Stars: General | ORDER G-MODES | stars: general | F-TYPE STARS | TO-CORE ROTATION | DELTA-SCUTI STARS | MAIN-SEQUENCE | stars: abundances | STELLAR ASTROPHYSICS MESA | ASTEROSEISMIC MEASUREMENT | EFFECTIVE TEMPERATURE | A-TYPE STARS | ASTRONOMY & ASTROPHYSICS | stars: chemically peculiar | FUNDAMENTAL PARAMETERS | stars: rotation
Journal Article
ASTRONOMY & ASTROPHYSICS, ISSN 1432-0746, 06/2019, Volume 626, p. A121
Helioseismology and asteroseismology of red giant stars have shown that distribution of angular momentum in stellar interiors, and the evolution of this...
HELIUM ABUNDANCE | CIRCULATION | stars: evolution | TO-CORE ROTATION | INTERNAL-ROTATION | MAIN-SEQUENCE | stars: oscillations | asteroseismology | ASTEROSEISMIC MEASUREMENT | STELLAR EVOLUTION | stars: statistics | ASTRONOMY & ASTROPHYSICS | GRAVITY MODES | TURBULENCE | DIFFUSION | stars: low-mass | stars: rotation | Solar and Stellar Astro
HELIUM ABUNDANCE | CIRCULATION | stars: evolution | TO-CORE ROTATION | INTERNAL-ROTATION | MAIN-SEQUENCE | stars: oscillations | asteroseismology | ASTEROSEISMIC MEASUREMENT | STELLAR EVOLUTION | stars: statistics | ASTRONOMY & ASTROPHYSICS | GRAVITY MODES | TURBULENCE | DIFFUSION | stars: low-mass | stars: rotation | Solar and Stellar Astro