42 citations · 114 across the 8 of their papers we have counts for
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Magnetic field geometry and magnetospheric environment of the strongly magnetic Of?p star NGC 1624-2
S. P. Järvinen, S. Hubrig, M. Schöller +3
NGC 1624-2 is an O7f?p star with a reported probable polar magnetic field strength 20 kG, which is the strongest magnetic field ever measured in an O-type star. We study the…
Cycle times of early M dwarf stars: mean field models versus observations
Manfred Küker, Günther Rüdiger, Katalin Oláh +1
Observations of early-type M stars suggest that there are two characteristic cycle times, one of order one year for fast rotators ( day) and another of order four…
A short and sudden increase of the magnetic field strength and the accompanying spectral variability in the O9.7V star HD54879
S. Hubrig, M. Kueker, S. P. Jarvinen +4
Only eleven O-type stars have been confirmed to possess large-scale organized magnetic fields. The presence of a -600G longitudinal magnetic field in the O9.7V star HD54879 with a…
Antisolar differential rotation of slowly rotating cool stars
G. Rüdiger, M. Küker, P. Käpylä +1
Rotating stellar convection transports angular momentum towards the equator, generating the characteristic equatorial acceleration of the solar rotation while the radial flux of an…
Cycle period, differential rotation and meridional flow for early M dwarf stars
M. Küker, G. Rüdiger, K. Oláh +1
Recent observations suggest the existence of two characteristic cycle times for early-type M stars dependent on the rotation period. They are of order one year for the fast rotator…
Analysing the effects of apodizing windows on local correlation tracking using Nirvana simulations of convection
Rohan E. Louis, B. Ravindra, Manolis K. Georgoulis +1
We employ different shapes of apodizing windows in the local correlation tracking (LCT) routine to retrieve horizontal velocities using numerical simulations of convection. LCT was…