Search Results - "Stello, D"

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    STRUCTURAL GLITCHES NEAR THE CORES OF RED GIANTS REVEALED BY OSCILLATIONS IN G-MODE PERIOD SPACINGS FROM STELLAR MODELS by Cunha, M. S., Stello, D., Avelino, P. P., Christensen-Dalsgaard, J., Townsend, R. H. D.

    Published in The Astrophysical journal (01-06-2015)
    “…ABSTRACT With recent advances in asteroseismology it is now possible to peer into the cores of red giants, potentially providing a way to study processes such…”
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    Measuring the vertical age structure of the Galactic disc using asteroseismology and SAGA by Casagrande, L, Aguirre, V Silva, Schlesinger, K J, Stello, D, Huber, D, Serenelli, A M, Schonrich, R, Cassisi, S, Pietrinferni, A, Hodgkin, S, Milone, A P, Feltzing, S, Asplund, M

    “…The existence of a vertical age gradient in the Milky Way disc has been indirectly known for long. Here, we measure it directly for the first time with seismic…”
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    Asteroseismic inference on rotation, gyrochronology and planetary system dynamics of 16 Cygni by Davies, G R, Chaplin, W J, Farr, W M, Garcia, R A, Lund, M N, Mathis, S, Metcalfe, T S, Appourchaux, T, Basu, S, Benomar, O, Campante, T L, Ceillier, T, Elsworth, Y, Handberg, R, Salabert, D, Stello, D

    “…The solar analogues 16 Cyg A and B are excellent asteroseismic targets in the Kepler field of view and together with a red dwarf and a Jovian planet form an…”
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    Analytical modelling of period spacings across the HR diagram by Cunha, M S, Avelino, P P, Christensen-Dalsgaard, J, Stello, D, Vrard, M, Jiang, C, Mosser, B

    “…ABSTRACT The characterization of stellar cores may be accomplished through the modelling of asteroseismic data from stars exhibiting either gravity-mode or…”
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    A Bayesian approach to scaling relations for amplitudes of solar-like oscillations in Kepler stars by Corsaro, E., Fröhlich, H.-E., Bonanno, A., Huber, D., Bedding, T. R., Benomar, O., De Ridder, J., Stello, D.

    “…We investigate different amplitude scaling relations adopted for the asteroseismology of stars that show solar-like oscillations. Amplitudes are among the most…”
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    PROBING THE DEEP END OF THE MILKY WAY WITH KEPLER: ASTEROSEISMIC ANALYSIS OF 854 FAINT RED GIANTS MISCLASSIFIED AS COOL DWARFS by Mathur, S., García, R. A., Huber, D., Regulo, C., Stello, D., Beck, P. G., Houmani, K., Salabert, D.

    Published in The Astrophysical journal (10-08-2016)
    “…ABSTRACT Asteroseismology has proven to be an excellent tool to determine not only global stellar properties with good precision, but also to infer the stellar…”
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    STRÖMGREN SURVEY FOR ASTEROSEISMOLOGY AND GALACTIC ARCHAEOLOGY: LET THE SAGA BEGIN by Casagrande, L, Aguirre, V Silva, STELLO, D, Huber, D, Serenelli, A M, Cassisi, S, Dotter, A, Milone, A P, Hodgkin, S, Marino, A F

    Published in The Astrophysical journal (01-06-2014)
    “…Asteroseismology has the capability of precisely determining stellar properties that would otherwise be inaccessible, such as radii, masses, and thus ages of…”
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    Characterization of red giant stars in the public Kepler data by Hekker, S., Gilliland, R. L., Elsworth, Y., Chaplin, W. J., De Ridder, J., Stello, D., Kallinger, T., Ibrahim, K. A., Klaus, T. C., Li, J.

    “…The first public release of long-cadence stellar photometric data collected by the NASA Kepler mission has now been made available. In this paper, we…”
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    ASTEROSEISMIC DETERMINATION OF OBLIQUITIES OF THE EXOPLANET SYSTEMS KEPLER-50 AND KEPLER-65 by Chaplin, W J, Sanchis-Ojeda, R, CAMPANTE, T L, Handberg, R, STELLO, D, Winn, J N, Basu, S, Christensen-Dalsgaard, J, Davies, G R, Metcalfe, T S

    Published in The Astrophysical journal (01-04-2013)
    “…Results on the obliquity of exoplanet host stars-the angle between the stellar spin axis and the planetary orbital axis-provide important diagnostic…”
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    Oscillating K Giants with the WIRE Satellite: Determination of Their Asteroseismic Masses by Stello, D, Bruntt, H, Preston, H, Buzasi, D

    Published in The Astrophysical journal (10-02-2008)
    “…Mass estimates of K giants are generally very uncertain. Traditionally, stellar masses of single field stars are determined by comparing their location in the…”
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