2017
Stars with a stable magnetic field: from pre-main sequence to compact remnants
JANÍK, Jan a Ernst PAUNZENZákladní údaje
Originální název
Stars with a stable magnetic field: from pre-main sequence to compact remnants
Název česky
Stars with a stable magnetic field: from pre-main sequence to compact remnants
Autoři
Vydání
2017
Další údaje
Jazyk
angličtina
Typ výsledku
Uspořádání konference
Obor
10308 Astronomy
Stát vydavatele
Česká republika
Utajení
není předmětem státního či obchodního tajemství
Odkazy
Organizační jednotka
Přírodovědecká fakulta
Klíčová slova česky
magnetické pole; hvězdy; bílí trpaslíci; neutronové hvězdy
Klíčová slova anglicky
magnetic field; stars; white dwarfs; neutron stars
Změněno: 17. 8. 2017 12:36, RNDr. Jan Janík, Ph.D.
V originále
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.
Česky
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.