Science, ISSN 0036-8075, 10/2013, Volume 342, Issue 6156, pp. 331 - 334
Stars hosting hot Jupiters are often observed to have high obliquities, whereas stars with multiple coplanar planets have been seen to have low obliquities....
Planets | Stars | REPORTS | Keplerian orbits | Star systems | Radial velocity | Stellar orbits | Astronomical transits | Planetary orbits | Inner planets | Astronomy | FNWI top publication | OBLIQUITIES | MODES | TRANSIT | ALIGNMENT | HOT STARS | MULTIDISCIPLINARY SCIENCES | EXOPLANETARY SYSTEMS | RED-GIANT STARS | PLANETARY SYSTEM | KEPLER | ROTATION AXIS | Observations | Extrasolar planets | Planetary systems | Orbits | Astrophysics | Solar systems | Stars & galaxies | Planes | Misalignment | Diagnostic systems | Dynamical systems
Planets | Stars | REPORTS | Keplerian orbits | Star systems | Radial velocity | Stellar orbits | Astronomical transits | Planetary orbits | Inner planets | Astronomy | FNWI top publication | OBLIQUITIES | MODES | TRANSIT | ALIGNMENT | HOT STARS | MULTIDISCIPLINARY SCIENCES | EXOPLANETARY SYSTEMS | RED-GIANT STARS | PLANETARY SYSTEM | KEPLER | ROTATION AXIS | Observations | Extrasolar planets | Planetary systems | Orbits | Astrophysics | Solar systems | Stars & galaxies | Planes | Misalignment | Diagnostic systems | Dynamical systems
Journal Article
Science, ISSN 0036-8075, 10/2015, Volume 350, Issue 6259, pp. 423 - 426
Internal stellar magnetic fields are inaccessible to direct observations, and little is known about their amplitude, geometry, and evolution. We demonstrate...
MIXED-MODES | SOLAR-LIKE OSCILLATIONS | CORE ROTATION | EVOLUTION | MULTIDISCIPLINARY SCIENCES | KEPLER | Space vehicles | Space ships | Magnetic fields | Observations | Red giants | Giant stars | Astrophysics | Red giant stars | Field strength | Stellar magnetic fields | Dipoles | Oscillations | Stellar oscillations | Vibration mode | Physics - Solar and Stellar Astrophysics | Sciences of the Universe
MIXED-MODES | SOLAR-LIKE OSCILLATIONS | CORE ROTATION | EVOLUTION | MULTIDISCIPLINARY SCIENCES | KEPLER | Space vehicles | Space ships | Magnetic fields | Observations | Red giants | Giant stars | Astrophysics | Red giant stars | Field strength | Stellar magnetic fields | Dipoles | Oscillations | Stellar oscillations | Vibration mode | Physics - Solar and Stellar Astrophysics | Sciences of the Universe
Journal Article
Nature, ISSN 0028-0836, 2012, Volume 481, Issue 7379, pp. 55 - 57
When the core hydrogen is exhausted during stellar evolution, the central region of a star contracts and the outer envelope expands and cools, giving rise to a...
CIRCULATION | OSCILLATIONS | MULTIDISCIPLINARY SCIENCES | ASTEROSEISMOLOGY | Measurement | Earth | Red giants | Stars | Research | Structure | Rotation | Natural history | Gravity | Spectrum analysis | Stars & galaxies | Astronomy | Physics - Solar and Stellar Astrophysics | Solar and Stellar Astrophysics | Sciences of the Universe | Astrophysics | Physics
CIRCULATION | OSCILLATIONS | MULTIDISCIPLINARY SCIENCES | ASTEROSEISMOLOGY | Measurement | Earth | Red giants | Stars | Research | Structure | Rotation | Natural history | Gravity | Spectrum analysis | Stars & galaxies | Astronomy | Physics - Solar and Stellar Astrophysics | Solar and Stellar Astrophysics | Sciences of the Universe | Astrophysics | Physics
Journal Article
4.
Full Text
A prevalence of dynamo-generated magnetic fields in the cores of intermediate-mass stars
Nature, ISSN 0028-0836, 01/2016, Volume 529, Issue 7586, pp. 364 - 367
Magnetic fields play a part in almost all stages of stellar evolution(1). Most low-mass stars, including the Sun, show surface fields that are generated by...
BRANCH | MODES | MULTIDISCIPLINARY SCIENCES | RED GIANT STARS | K-GIANTS | KEPLER | ASTEROSEISMOLOGY | Star formation | Magnetic fields | Observations | Helium | Star & galaxy formation | Stars & galaxies | Physics - Solar and Stellar Astrophysics
BRANCH | MODES | MULTIDISCIPLINARY SCIENCES | RED GIANT STARS | K-GIANTS | KEPLER | ASTEROSEISMOLOGY | Star formation | Magnetic fields | Observations | Helium | Star & galaxy formation | Stars & galaxies | Physics - Solar and Stellar Astrophysics
Journal Article
The Astrophysical Journal, ISSN 1538-4357, 10/2019, Volume 884, Issue 2, p. 107
Journal Article
The Astrophysical Journal, ISSN 1538-4357, 06/2019, Volume 878, Issue 2, p. 136
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 03/2018, Volume 475, Issue 1, pp. 981 - 998
Stellar models rely on a number of free parameters. High-quality observations of eclipsing binary stars observed by Kepler offer a great opportunity to...
Stars: evolution | Stars: oscillations | stars: oscillations | stars: evolution | ASTRONOMY & ASTROPHYSICS | SOLAR | RATIO | 3D CONVECTION SIMULATIONS | OSCILLATIONS | Eclipsing binary stars | Red giant stars | Oscillation modes | Stellar seismology | Data analysis | Parameters | Convective mixing | Binary stars | Stellar evolution | Modelling | Mathematical models | Calibration | Physics - Solar and Stellar Astrophysics
Stars: evolution | Stars: oscillations | stars: oscillations | stars: evolution | ASTRONOMY & ASTROPHYSICS | SOLAR | RATIO | 3D CONVECTION SIMULATIONS | OSCILLATIONS | Eclipsing binary stars | Red giant stars | Oscillation modes | Stellar seismology | Data analysis | Parameters | Convective mixing | Binary stars | Stellar evolution | Modelling | Mathematical models | Calibration | Physics - Solar and Stellar Astrophysics
Journal Article
Astrophysical Journal, Supplement Series, ISSN 0067-0049, 09/2013, Volume 208, Issue 1, pp. 4 - 43
We substantially update the capabilities of the open source software package Modules for Experiments in Stellar Astrophysics (MESA), and its one-dimensional...
planets and satellites: physical evolution | stars: massive | asteroseismology | methods: numerical | stars: evolution | stars: rotation | ANGULAR-MOMENTUM TRANSPORT | PRESUPERNOVA EVOLUTION | WHITE-DWARFS | INTERNAL-ROTATION | DIFFERENTIAL ROTATION | WOLF-RAYET STARS | EQUATION-OF-STATE | ASTRONOMY & ASTROPHYSICS | ZZ-CETI STARS | THERMOHALINE CONVECTION | LARGE-MAGELLANIC-CLOUD | Mesas | Adiabatic flow | Software packages | Astrophysics | Planetary evolution | Modules | Stars | Mathematical models | Source code | ROTATION | REACTION KINETICS | NUCLEAR REACTIONS | OPACITY | ONE-DIMENSIONAL CALCULATIONS | SUPERNOVAE | ABUNDANCE | BOUNDARY CONDITIONS | ANGULAR MOMENTUM | NUCLEI | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | COOLING | STAR EVOLUTION | SCALING | HELIUM BURNING | WHITE DWARF STARS | COMPUTER CODES | EQUATIONS OF STATE | COSMIC GAMMA BURSTS | OSCILLATIONS | PULSATIONS | STAR MODELS
planets and satellites: physical evolution | stars: massive | asteroseismology | methods: numerical | stars: evolution | stars: rotation | ANGULAR-MOMENTUM TRANSPORT | PRESUPERNOVA EVOLUTION | WHITE-DWARFS | INTERNAL-ROTATION | DIFFERENTIAL ROTATION | WOLF-RAYET STARS | EQUATION-OF-STATE | ASTRONOMY & ASTROPHYSICS | ZZ-CETI STARS | THERMOHALINE CONVECTION | LARGE-MAGELLANIC-CLOUD | Mesas | Adiabatic flow | Software packages | Astrophysics | Planetary evolution | Modules | Stars | Mathematical models | Source code | ROTATION | REACTION KINETICS | NUCLEAR REACTIONS | OPACITY | ONE-DIMENSIONAL CALCULATIONS | SUPERNOVAE | ABUNDANCE | BOUNDARY CONDITIONS | ANGULAR MOMENTUM | NUCLEI | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | COOLING | STAR EVOLUTION | SCALING | HELIUM BURNING | WHITE DWARF STARS | COMPUTER CODES | EQUATIONS OF STATE | COSMIC GAMMA BURSTS | OSCILLATIONS | PULSATIONS | STAR MODELS
Journal Article
9.
Full Text
Gravity modes as a way to distinguish between hydrogen- and helium-burning red giant stars
Nature, ISSN 0028-0836, 2011, Volume 471, Issue 7340, pp. 608 - 611
Red giants are evolved stars that have exhausted the supply of hydrogenin their cores and instead burn hydrogen in a surrounding shell(1,2). Once a red giant...
STELLAR OSCILLATIONS | CODE | MULTIDISCIPLINARY SCIENCES | MASS | SOLAR-LIKE OSCILLATIONS | COROT | KEPLER | ASTEROSEISMOLOGY | Research | Helium | Observations | Hydrogen | Red giants | Spectrum allocation | Gravity | Red giant stars | Spacecraft | Oscillations | Shells | Tools | Combustion | Burns | Physics - Solar and Stellar Astrophysics | Solar and Stellar Astrophysics | Sciences of the Universe | Astrophysics | Physics
STELLAR OSCILLATIONS | CODE | MULTIDISCIPLINARY SCIENCES | MASS | SOLAR-LIKE OSCILLATIONS | COROT | KEPLER | ASTEROSEISMOLOGY | Research | Helium | Observations | Hydrogen | Red giants | Spectrum allocation | Gravity | Red giant stars | Spacecraft | Oscillations | Shells | Tools | Combustion | Burns | Physics - Solar and Stellar Astrophysics | Solar and Stellar Astrophysics | Sciences of the Universe | Astrophysics | Physics
Journal Article
Science, ISSN 0036-8075, 8/2012, Volume 337, Issue 6094, pp. 556 - 559
In the solar system, the planets' compositions vary with orbital distance, with rocky planets in close orbits and lower-density gas giants in wider orbits. The...
Stellar masses | Planets | Extrasolar planets | Stars | REPORTS | Keplerian orbits | Stellar orbits | Astronomical transits | Astronomical research | Planetary orbits | Planetary composition | FNWI top publication | LOW-MASS | STAR | TRANSIT TIMING VARIATIONS | MISSION | PERFORMANCE | STABILITY | MULTIDISCIPLINARY SCIENCES | SYSTEMS | SCIENCE | COMPANION | CURVES | Orbits | Research | Natural history | Planetology | Astronomy | Neptune | Gas giant planets | Space telescopes | Solar system | Density | Physics - Earth and Planetary Astrophysics | ASTRONOMY AND ASTROPHYSICS
Stellar masses | Planets | Extrasolar planets | Stars | REPORTS | Keplerian orbits | Stellar orbits | Astronomical transits | Astronomical research | Planetary orbits | Planetary composition | FNWI top publication | LOW-MASS | STAR | TRANSIT TIMING VARIATIONS | MISSION | PERFORMANCE | STABILITY | MULTIDISCIPLINARY SCIENCES | SYSTEMS | SCIENCE | COMPANION | CURVES | Orbits | Research | Natural history | Planetology | Astronomy | Neptune | Gas giant planets | Space telescopes | Solar system | Density | Physics - Earth and Planetary Astrophysics | ASTRONOMY AND ASTROPHYSICS
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 08/2017, Volume 469, Issue 4, pp. 4578 - 4583
In the power spectra of oscillating red giants, there are visually distinct features defining stars ascending the red giant branch from those that have...
asteroseismology | methods: data analysis | stars: oscillations | techniques: image processing | stars: statistics | ASTRONOMY & ASTROPHYSICS | RED GIANTS | MIXED-MODES | SPECTRA
asteroseismology | methods: data analysis | stars: oscillations | techniques: image processing | stars: statistics | ASTRONOMY & ASTROPHYSICS | RED GIANTS | MIXED-MODES | SPECTRA
Journal Article
Astrophysical Journal, ISSN 0004-637X, 08/2014, Volume 790, Issue 2, pp. 127 - 21
The Sloan Digital Sky Survey III's Apache Point Observatory Galactic Evolution Experiment (APOGEE) is a high-resolution near-infrared spectroscopic survey...
Galaxy: stellar content | Galaxy: disk | Galaxy: structure | stars: general | Galaxy: abundances | stars: distances | GALACTIC DISK | POPULATION SYNTHESIS | ABSOLUTE MAGNITUDE | SKY SURVEY 2MASS | STELLAR EVOLUTION DATABASE | WAY DISK | ASTRONOMY & ASTROPHYSICS | MODEL ATMOSPHERES | LARGE-MAGELLANIC-CLOUD | GIANT STARS | OPEN CLUSTERS | Metallicity | Stars | Disks | Mathematical models | Apogees | Glass transition temperature | Catalogs | Sun | Physics - Astrophysics of Galaxies | Physics | Astrophysics | LUMINOSITY | DISTANCE | APPROXIMATIONS | DUSTS | CATALOGS | GALACTIC EVOLUTION | METALLICITY | SUN | ABUNDANCE | ISOCHRONOUS CYCLOTRONS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | STAR EVOLUTION | COLOR | PHOTOMETRY | SPACE DEPENDENCE | GRAVITATION | PROPER MOTION | MILKY WAY | SPECTRA | SURFACES
Galaxy: stellar content | Galaxy: disk | Galaxy: structure | stars: general | Galaxy: abundances | stars: distances | GALACTIC DISK | POPULATION SYNTHESIS | ABSOLUTE MAGNITUDE | SKY SURVEY 2MASS | STELLAR EVOLUTION DATABASE | WAY DISK | ASTRONOMY & ASTROPHYSICS | MODEL ATMOSPHERES | LARGE-MAGELLANIC-CLOUD | GIANT STARS | OPEN CLUSTERS | Metallicity | Stars | Disks | Mathematical models | Apogees | Glass transition temperature | Catalogs | Sun | Physics - Astrophysics of Galaxies | Physics | Astrophysics | LUMINOSITY | DISTANCE | APPROXIMATIONS | DUSTS | CATALOGS | GALACTIC EVOLUTION | METALLICITY | SUN | ABUNDANCE | ISOCHRONOUS CYCLOTRONS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | STAR EVOLUTION | COLOR | PHOTOMETRY | SPACE DEPENDENCE | GRAVITATION | PROPER MOTION | MILKY WAY | SPECTRA | SURFACES
Journal Article