activity
20042008
most citedToroidal versus poloidal magnetic fields in Sun-like stars: a rotation threshold

275 citations · 279 across the 9 of their papers we have counts for

collaborators
Showing 2007Show all

6 papers · 1 filter

astro-ph2007

Why are some A stars magnetic, while most are not?

G. A. Wade, J. Silvester, K. Bale +21

A small fraction of intermediate-mass main sequence (A and B type) stars have strong, organised magnetic fields. The large majority of such stars, however, show no evidence for mag…

astro-ph2007

Magnetism and rotation in Herbig Ae/Be stars

E. Alecian, G. A. Wade, C. Catala +8

Among the main sequence intermediate mass A and B stars, around 5% host large-scale organized magnetic fields. Most of these stars are very slow rotators compared to their non-magn…

astro-ph2007

Spectropolarimetry of cool stars

P. Petit

In recent years, the development of spectropolarimetric techniques deeply modified our knowledge of stellar magnetism. In the case of solar-type stars, the challenge is to measure…

astro-ph20071 cited

Detection of the Molecular Zeeman Effect in Circular Polarization on Cool Active Stars

S. V. Berdyugina, P. Petit, D. M. Fluri +2

We report on the first ever detection of circular polarization in molecular lines forming in magnetic regions on the surfaces of active stars. The new observations were obtained wi…

astro-ph20071 cited

First Direct Detection of Magnetic Fields in Starspots and Stellar Chromospheres

S. V. Berdyugina, D. M. Fluri, N. Afram +5

Here we report on the first detection of circular polarization in molecular lines formed in cool magnetic regions (starspots) and in chromospheric emission lines formed in hot plag…

astro-ph20072 cited

Magnetic topologies of cool stars

J. -F. Donati, M. M. Jardine, P. Petit +14

Stellar magnetic fields can be investigated using several, very complementary approaches. While conventional spectroscopy is capable of estimating the average magnetic strength of…