Stars with a stable magnetic field: from pre-main sequence to compact remnants
Magnetic fields play an important role in the evolution of all stellar objects, through their ability to influence and alter the angular momentum evolution, internal mixing, activity phenomena, surface abundances and mass-loss of stars. This research field benefits from new highly accurate measurements and numerical simulations, enabling stellar astrophysicists to take magnetic fields into account in most models of stellar structure and evolution. We want to bring together researchers from different fields where magnetic fields play an important role to join their efforts and discuss their common interests.

When:   August 28 - September 01, 2017

Where:  Brno, Czech Republic





21.11.2017: Proceedings final deadline: 11.12.2017
19.09.2017: Proceedings deadline: 10.11.2017
06.09.2017: Conference pictures
30.08.2017: The conference photo
01.07.2017: The deadline for the submission of abstracts was extended to 15.07.2017
12.06.2017: The conference poster
21.03.2017: The registration is now open
20.03.2017: Update of the Programme
21.10.2016: Preliminary release of the Conference Website.