Showing 61 - 80 results of 211 for search '"asteroseismology"', query time: 0.12s Refine Results
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    WHAT ASTEROSEISMOLOGY CAN DO FOR EXOPLANETS: KEPLER-410A b IS A SMALL NEPTUNE AROUND A BRIGHT STAR, IN AN ECCENTRIC ORBIT CONSISTENT WITH LOW OBLIQUITY by Van Eylen, V., Lund, Mikkel N., Aguirre, V. Silva, Arentoft, T., Kjeldsen, H., Albrecht, Simon H., Chaplin, William J., Isaacson, Howard, Pedersen, M. G., Jessen-Hansen, J., Tingley, B., Christensen-Dalsgaard, J., Aerts, C., Campante, T. L., Bryson, Stephen T.

    Published 2015
    “…We determine via asteroseismology the following stellar and planetary parameters with high precision; M [subscript *] = 1.214 ± 0.033 M ☉, R [subscript *] = 1.352 ± 0.010 R ☉, age =2.76 ± 0.54 Gyr, planetary radius (2.838 ± 0.054 R ⊕), and orbital eccentricity (0.17[+0.07 over -0.06]). …”
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    Article
  17. 77

    Modelling Neutron-Star Ocean Dynamics by Fabian Gittins, Thomas Celora, Aru Beri, Nils Andersson

    Published 2023-05-01
    Subjects: “…asteroseismology…”
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