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  • Raphaëlle D. Haywood
    978-3-319-41273-3
    2016
    Edition 1
    • Nominated as an outstanding Ph.D. thesis by the University of St. Andrews, UK
    • Includes clear explanations, making it easy to read and accessible to a broad audience with minimum scientific background knowledge
    • Presents a new, state-of-the-art technique that is expected to become mainstream in planet-hunting research over the next few years
    • Demonstrates that the radial-velocity variations mainly arise from suppression of photospheric convection by magnetic fields. This finding represents a significant step towards measuring the masses of potentially habitable planets orbiting Sun-like stars
    • Includes supplementary material: sn.pub/extras

    €180

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