Publicaciones en las que colabora con ANDRÉS MOYA BEDÓN (19)

2012

  1. Pulsation spectrum of δ Scuti stars: The binary HD 50870 as seen with CoRoT and HARPS

    Astronomy and Astrophysics, Vol. 542

2010

  1. Age determination of the HR8799 planetary system using asteroseismology

    Monthly Notices of the Royal Astronomical Society: Letters

  2. The planetary system host HR 8799: On its λ Bootis nature

    Monthly Notices of the Royal Astronomical Society, Vol. 406, Núm. 1, pp. 566-575

2009

  1. Asteroseismic analysis of the CoRoT δ Scuti star HD174936

    Astronomy and Astrophysics, Vol. 506, Núm. 1, pp. 79-83

  2. Asteroseismological modeling of the multiperiodic λ bootis star 29 cygni

    Astrophysical Journal, Vol. 697, Núm. 1, pp. 522-534

  3. HD 50844: A new look at ä Scuti stars from CoRoT space photometry

    Astronomy and Astrophysics, Vol. 506, Núm. 1, pp. 85-93

  4. On the λ Bootis nature: The case of 29 Cygni

    AIP Conference Proceedings

  5. The tip of the iceberg: The frequency content of the δ Sct star HD 50844 from CoRoT space photometry

    AIP Conference Proceedings

2008

  1. A procedure for modelling asymptotic g-mode pulsators: The case of γ Doradus stars

    Astronomische Nachrichten

  2. The limits of validity of the Frequency Ratio Method: The particular case of γ Doradus stars

    Astronomische Nachrichten

  3. γ Doradus variable stars in the Pleiades cluster: Results from a photometric multiste campaign

    Journal of Physics: Conference Series

2007

  1. Asteroseismology with the WIRE satellite I. Combining ground- And space-based photometry of the δ Scuti star ε Cephei

    Astronomy and Astrophysics, Vol. 461, Núm. 2, pp. 619-630

  2. The field high-amplitude SX Phoenicis variable BL camelopardalis: Results from a multisite photometric campaign I. Pulsation

    Astronomy and Astrophysics, Vol. 471, Núm. 1, pp. 255-264

2006

  1. HD 172189, a cluster member binary system with a δ Scuti component in the field of view of COROT

    Astrophysics and Space Science

  2. The frequency ratio method and the new multiperiodic γ Doradus star HD 218427

    Astronomy and Astrophysics, Vol. 450, Núm. 2, pp. 715-723

2005

  1. Frequency ratio method for seismic modeling of γ Doradus stars

    Astronomy and Astrophysics, Vol. 432, Núm. 1, pp. 189-198

  2. Frequency ratio method for seismic modelling of γ Doradus stars II. The role of rotation

    Astronomy and Astrophysics, Vol. 443, Núm. 1, pp. 271-282

  3. HD 172189: An eclipsing and spectroscopic binary with a δ Sct-type pulsating component in an open cluster

    Astronomy and Astrophysics, Vol. 440, Núm. 2, pp. 711-714

2004

  1. The pre-main-sequence star HD 34282: A very short-period δ Scuti-type pulsator

    Monthly Notices of the Royal Astronomical Society, Vol. 352, Núm. 2