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Radial-velocity Searches for Planets Around Active Stars

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 €162
10% OFF

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