96 citations · 404 across the 9 of their papers we have counts for
9 papers
A magnetic field study of two fast-rotating, radio bright M dwarfs. StKM 1-1262 and V374 Peg
S. Bellotti, P. I. Cristofari, J. R. Callingham +8
Radio observations at low frequencies are sensitive to the magnetic activity of stars and the plasma environment surrounding them. The accurate interpretation of the processes unde…
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…
Linking chromospheric activity and magnetic field properties for late-type dwarf stars
E. L. Brown, S. V. Jeffers, S. C. Marsden +9
Spectropolarimetric data allow for simultaneous monitoring of stellar chromospheric activity and the surface-averaged longitudinal magnetic field, $B_l…
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…
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…
A hot Jupiter around the very active weak-line T Tauri star TAP 26
L. Yu, J. -F. Donati, E. M. Hébrard +17
We report the results of an extended spectropolarimetric and photometric monitoring of the weak-line T Tauri star TAP 26, carried out within the MaTYSSE programme with the ESPaDOnS…
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…
Ionisation in atmospheres of Brown Dwarfs and extrasolar planets I The role of electron avalanche
Ch. Helling, M. Jardine, S. Witte +1
Brown Dwarf and extrasolar planet atmospheres form clouds which strongly influence the local chemistry and physics. These clouds are globally neutral obeying dust-gas charge equili…
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…