ALMA reveals a large structured disk and nested rotating outflows in DG Tauri B

At small Reynolds numbers, before the flow transition from convective to absolute instability, fluctuations start rising at the edge, within a region where the flow is no longer

At small Reynolds numbers, before the flow transition from convective to absolute instability, fluctuations start rising at the edge, within a region where the flow is no longer

Hishida [17] revealed the asymptotic be- havior of the stationary Stokes flow around a rotating obstacle, and showed that the rotation of the obstacle leads to the resolution of

Scattered light images of transition disks (disks with an inner dust depleted cavity) show clear evidence for misaligned inner regions, either with narrow shadow lanes in the outer

The focus was on the influence of the rotation rate on the mean flow, turbulence, and heat transfer in the axisymmetric wall jet developing along the disk outside the

Our Cycle 4 ALMA data reveal a rotating wide-angle flow in SO and SO 2 around the SiO jet with a mean speed of ∼30 km s −1 and an onion-like velocity structure filling in the base

The context of the analysis is the following : (1) the detuning is taken into account by voluntarily breaking the cyclic symmetry of the structure with the use of a pattern

The enhanced frequency dispersion associated with coupled charging and faradaic currents is seen by examination of the global interfacial impedance for the APS and NAPS cases, shown