Showing 1–20 of 25 results
/ Date/ Name
Mar 20, 2020Accretion in low-mass members of the Orion Nebula Cluster with young transition disksAug 4, 2012Velocity asymmetries in YSO jets: Intrinsic and extrinsic mechanismsMay 26, 2009Two-component jet simulations: Combining analytical and numerical approachesMay 21, 2009Two-component jet simulations: II. Combining analytical disk and stellar MHD outflow solutionsJul 13, 2022Double flows anchored in a Kerr black hole horizon. I. Meridionally self-similar MHD models with loading termsJul 6, 2004Relativistic Parker winds with variable effective polytropic indexJun 22, 2007Two-flow magnetohydrodynamical jets around young stellar objectsOct 14, 2012Counterrotation in magnetocentrifugally driven jets and other windsFeb 25, 2016Modelling stellar jets with magnetospheres using as initial states analytical MHD solutionsJun 7, 1999Nonradial and nonpolytropic astrophysical outflows IV. Magnetic or thermal collimation of winds into jets?Dec 15, 2017Nonradial and nonpolytropic astrophysical outflows. X. Relativistic MHD rotating spine jets in Kerr metricJul 13, 2011Nonradial and nonpolytropic astrophysical outflows IX. Modeling T Tauri jets with a low mass-accretion rateJun 10, 2010Relativistic spine jets from Schwarzschild black holes: "Application to AGN radioloud sources"Oct 20, 2005Nonradial and nonpolytropic astrophysical outflows VIII. A GRMHD generalization for relativistic jetsAug 28, 2006Two-component magnetohydrodynamical outflows around young stellar objects Interplay between stellar magnetospheric winds and disc-driven jetsAug 31, 2001Jet Formation and Collimation in AGN and microQuasarsMay 14, 2002Nonradial and nonpolytropic astrophysical outflows. V. Acceleration and collimation of self-similar windsJun 16, 2022Nonradial and nonpolytropic astrophysical outflows. XI. Simulations of the circumstellar environment of RY TauDec 16, 2013Young stellar object jet models: From theory to synthetic observationsMay 30, 2017Shocks in relativistic transverse stratified jets, a new paradigm for radio-loud AGN