ANDRES
MOYA SIMARRO
CATEDRÁTICO/A DE UNIVERSIDAD
Université de Toulouse
Tolosa, FranciaPublicaciones en colaboración con investigadores/as de Université de Toulouse (13)
2013
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An in-depth study of HD 174966 with CoRoT photometry and HARPS spectroscopy: Large separation as a new observable for δ Scuti stars
Astronomy and Astrophysics, Vol. 559
2011
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The Kepler characterization of the variability among A-and F-type stars: I. General overview
Astronomy and Astrophysics, Vol. 534
2010
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A precise asteroseismic age and radius for the evolved sun-like star KIC 11026764
Astrophysical Journal, Vol. 723, Núm. 2, pp. 1583-1598
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Has a star enough energy to excite the thousand of modes observed with CoRoT?
Astrophysical Journal Letters, Vol. 710, Núm. 1 PART 2
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Mode trapping in sdO models
Astrophysics and Space Science, Vol. 329, Núm. 1, pp. 205-209
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Study of sdO models: Mode trapping
Monthly Notices of the Royal Astronomical Society, Vol. 403, Núm. 4, pp. 1983-1992
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Study of sdO models: Pulsation analysis
Monthly Notices of the Royal Astronomical Society, Vol. 402, Núm. 1, pp. 295-306
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The asteroseismic potential of kepler: First results for solar-type stars
Astrophysical Journal Letters, Vol. 713, Núm. 2 PART 2
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The rapidly pulsating sdO star, SDSS J160043.6+074802.9
Monthly Notices of the Royal Astronomical Society, Vol. 401, Núm. 1, pp. 23-34
2009
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Ground-based observations of the β Cephei CoRoT main target HD180 642: Abundance analysis and mode identification
Astronomy and Astrophysics, Vol. 506, Núm. 1, pp. 269-280
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HD 172189: Another step in furnishing one of the best laboratories known for asteroseismic studies
Astronomy and Astrophysics, Vol. 507, Núm. 2, pp. 901-910
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Radius determination of solar-type stars using asteroseismology: What to expect from the kepler mission
Astrophysical Journal, Vol. 700, Núm. 2, pp. 1589-1602
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Seismology of β Cephei stars: Differentially rotating models for interpreting the oscillation spectrum of ν Eridani
Astrophysical Journal, Vol. 690, Núm. 2, pp. 1401-1411