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Gravity modes as a way to distinguish between hydrogen- and helium-burning red giant stars

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
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Gravity modes in rapidly rotating polytropic stars

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
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Gravity modes in rapidly rotating stars. Limits of perturbative methods

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
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GREAT [CII] and CO observations of the BD+40°4124 region

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
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Green's functions for far-side seismic images: a polar expansion approach

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
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Grids of ATLAS9 Model Atmospheres and MOOG Synthetic Spectra

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Grids of stellar models with rotation - I. Models from 0.8 to 120 Msun at solar metallicity (Z = 0.014)

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
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Grids of stellar models with rotation II. WR populations and supernovae/GRB progenitors at Z = 0.014

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Gross-Pitaevskii model of pulsar glitches

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Ground-Based Astrometry 2010-2020

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
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Ground-Based BVRI Follow-Up Observations of the Cepheid V1154 Cyg in Kepler's Field

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Ground-based follow-up in relation to Kepler Asteroseismic Investigation

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Ground-based measurements of solar diameter

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
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Ground-based observations of Kepler asteroseismic targets

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Ground-based observations of the beta Cephei CoRoT main target HD 180642: abundance analysis and mode identification

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
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Ground-based photometry of space-based transit detections: Photometric follow-up of the CoRoT mission

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Growing electrostatic modes in the isothermal pair plasma of the pulsar magnetosphere

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
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Growing transverse oscillations of a multistranded loop observed by SDO/AIA

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Growth of the MRI in Accretion Discs -- the Influence of Radiation Transport

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Growth rate of small-scale dynamo at low magnetic Prandtl numbers

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