activity
20072022
most citedThe shocking transit of WASP-12b: Modelling the observed early ingress in the near ultraviolet

96 citations · 204 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR20227 cited

Can scallop-shell stars trap dust in their magnetic fields?

Hannah Sanderson, Moira Jardine, Andrew Collier Cameron +2

One of the puzzles to have emerged from the Kepler and TESS missions is the existence of unexplained dips in the lightcurves of a small fraction of rapidly-rotating M dwarfs in you…

astro-ph.SR202223 cited

MOVES V. Modelling star-planet magnetic interactions of HD 189733

A. Strugarek, R. Fares, V. Bourrier +10

Magnetic interactions between stars and close-in planets may lead to a detectable signal on the stellar disk. HD 189733 is one of the key exosystems thought to harbor magnetic inte…

astro-ph.SR202226 cited

The crucial role of surface magnetic fields for stellar dynamos: Epsilon Eridani, 61 Cygni A, and the Sun

S. V. Jeffers, R. H. Cameron, S. C. Marsden +9

Cool main-sequence stars, such as the Sun, have magnetic fields which are generated by an internal dynamo mechanism. In the Sun, the dynamo mechanism produces a balance between the…

astro-ph.EP201196 cited

The shocking transit of WASP-12b: Modelling the observed early ingress in the near ultraviolet

J. Llama, K. Wood, M. Jardine +4

Near ultraviolet observations of WASP-12b have revealed an early ingress compared to the optical transit lightcurve. This has been interpreted as due to the presence of a magnetosp…

astro-ph200752 cited

Why are accreting T Tauri stars observed to be less luminous in X-rays than non-accretors?

S. G. Gregory, K. Wood, M. Jardine

Accreting T Tauri stars are observed to be less luminous in X-rays than non-accretors, an effect that has been detected in various star forming regions. To explain this we have com…