Theory of fossil magnetic field

Abstract

Theory of fossil magnetic field is based on the observations, analytical estimations and numerical simulations of magnetic flux evolution during star formation in the magnetized cores of molecular clouds. Basic goals, main features of the theory and manifestations of MHD effects in young stellar objects are discussed.

arXiv comment18 pages, accepted for publication in Advances in Space Research (2014)

References in corpus (12)

• Rosseland and Planck Mean Opacities for Protoplanetary Discs
• Magnetic Fields in the Formation of Sun-Like Stars
• SCUBA Polarization Measurements of the Magnetic Field Strengths in the L183, L1544, and L43 Prestellar Cores
• Heat and Dust in Active Layers of Protostellar Disks
• Anchoring Magnetic Field in Turbulent Molecular Clouds
• Alignment Between Flattened Protostellar Infall Envelopes and Ambient Magnetic Fields
• The nonisothermal stage of magnetic star formation. II. Results
• Magnetically Controlled Spasmodic Accretion During Star Formation. II. Results
• Fossil magnetic field of accretion disks of young stars
• Magnetically Controlled Spasmodic Accretion During Star Formation. I. Formulation of the Problem and Method of Solution
• On the magnetic flux problem in star formation
• Magnetism in pre-MS intermediate-mass stars and the fossil field hypothesis

Cited by in corpus (9)

• Do A-type stars flare?
• Gravity waves in strong magnetic fields
• Large-scale magnetic field in the accretion discs of young stars: the influence of magnetic diffusion, buoyancy and Hall effect
• Dynamics of magnetic flux tubes and IR-variability of Young Stellar Objects
• Magnetic field buoyancy in accretion disks of young stars
• Dynamics of magnetic flux tubes in accretion discs of T Tauri stars
• Dynamics of magnetized accretion disks of young stars
• Influence of Ohmic and ambipolar heating on thermal structure of accretion discs
• Physical and chemical vertical structure of magnetostatic accretion disks of young stars