New simulations show that interactions with a magnetic field can work to decrease the distance between still forming binary protostars. These results can help explain the characteristics of the binary ...
In this picture, the binary does not simply plow through surrounding gas and gradually slow down. Instead, the gas is tied to large-scale magnetic field lines that connect the inner disk to the outer ...
Visualization of gas flows around a binary protostar system calculated by ATERUI III. The gas shown in red orbits around one of the two protostars. The gas shown in blue orbits around the combined ...
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