text: 189,7,1279239019541532672,384900803,Shantanu Basu,New paper on gravitational collapse and star formation with misaligned magnetic and rotation axes. Misalignment leads to larger disks and weaker outflows and complex magnetic field patterns. <LINK> @westernuPhysAst @KyushuUniv_EN #KagoshimaUniversity <LINK>,https://arxiv.org/abs/2006.13233,"The formation of circumstellar disks is investigated using three-dimensional resistive magnetohydrodynamic simulations, in which the initial prestellar cloud has a misaligned rotation axis with respect to the magnetic field. We examine the effects of (i) the initial angle difference between the global magnetic field and the cloud rotation axis ($\theta_0$) and (ii) the ratio of the thermal to gravitational energy ($\alpha_0$). We study $16$ models in total and calculate the cloud evolution until $\sim \! 5000$ yr after protostar formation. Our simulation results indicate that an initial non-zero $\theta_0$ ($> 0$) promotes the disk formation but tends to suppress the outflow driving, for models that are moderately gravitationally unstable, $\alpha_0 \lesssim 1$. In these models, a large-sized rotationally-supported disk forms and a weak outflow appears, in contrast to a smaller disk and strong outflow in the aligned case ($\theta_0 = 0$). Furthermore, we find that when the initial cloud is highly unstable with small $\alpha_0$, the initial angle difference $\theta_0$ does not significantly affect the disk formation and outflow driving. ","The Effect of Misalignment between Rotation Axis and Magnetic Field on