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  1. No Access

    Article

    The excitation of solar-like oscillations in a δ Sct star by efficient envelope convection

    Delta Scuti (δ Sct)1 stars are opacity-driven pulsators with masses of 1.5–2.5M⊙, their pulsations resulting from the varying ionization of helium. In less massive stars2 such as the Sun, convection transports ma...

    V. Antoci, G. Handler, T. L. Campante, A. O. Thygesen, A. Moya, T. Kallinger… in Nature (2011)

  2. Article

    Erratum to: “Exoplanet discoveries with the CoRoT space observatory”

    H. Lammer, R. Dvorak, M. Deleuil, P. Barge, H. J. Deeg, C. Moutou… in Solar System Research (2011)

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  3. No Access

    Article

    Exoplanet discoveries with the CoRoT space observatory

    The CoRoT space observatory is a project which is led by the French space agency CNES and leading space research institutes in Austria, Brazil, Belgium, Germany and Spain and also the European Space Agency ESA...

    H. Lammer, R. Dvorak, M. Deleuil, P. Barge, H. J. Deeg, C. Moutou… in Solar System Research (2010)

  4. No Access

    Article

    A transiting giant planet with a temperature between 250 K and 430 K

    About 70 of the more than 400 known extrasolar planets transit their central star, making it possible to observe their atmospheres and determine various key parameters. The transiting extra-solar planets so fa...

    H. J. Deeg, C. Moutou, A. Erikson, Sz. Csizmadia, B. Tingley, P. Barge, H. Bruntt… in Nature (2010)

  5. No Access

    Article

    Late-Type Active Stars: Rotation & Companions

    Rapid rotation has been established empirically as the controlling factor for the magnetic field strength and the magnetic activity level of single late-type (F-M) stars. The dynamo theories explain this fact ...

    T. H. Dall, K. G. Strassmeier, H. Bruntt in Astrophysics and Space Science (2006)

  6. No Access

    Chapter

    Late-Type Active Stars: Rotation & Companions

    Rapid rotation has been established empirically as the controlling factor for the magnetic field strength and the magnetic activity level of single late-type (F-M) stars. The dynamo theories explain this fact ...

    T. H. Dall, K. G. Strassmeier, H. Bruntt in Close Binaries in the 21st Century: New Op… (2006)

  7. No Access

    Chapter and Conference Paper

    Abundance Variations in NGC 288, NGC 362 and NGC 1851

    Strömgren uvby photometry is a powerful tool to study abundance variations in globular clusters through the c 1 and m 1 indices. This is because the NH (3360Å) and ...

    F. Grundahl, H. Bruntt in Chemical Abundances and Mixing in Stars in… (2006)

  8. No Access

    Chapter and Conference Paper

    Studying Old Open Clusters with Detached Eclipsing Binaries

    The single most important parameter which determines the evolution of a star is its mass. Detached eclipsing binaries offer the possibility to determine accurate masses and radii for their components. By study...

    F. Grundahl, S. Meibom, H. Bruntt… in Chemical Abundances and Mixing in Stars in… (2006)

  9. No Access

    Article

    Giant Vibrations in Dip

    This work reports the discovery of solar-type oscillations in thegiant star ξ Hydrae.

    T.C. Teixeira, J. Christensen-Dalsgaard, F. Carrier… in Astrophysics and Space Science (2003)

  10. No Access

    Chapter and Conference Paper

    Giant Vibrations in Dip

    This work reports the discovery of solar-type oscillations in the giant star ξ Hydrae.

    T. C. Teixeira, J. Christensen-Dalsgaard… in Asteroseismology Across the HR Diagram (2003)