Abstract
The thermomagnetic torque, known to exist when a gas of polyatomic molecules experiences a temperature gradient in the presence of a magnetic field, has been investigated as a possible source of stellar rotational angular momentum. The effect does not appear to be significant during pre-mainsequence evolution. To influence stellar rotation a process must be capable of generating torques on the order of 1040 dyn cm−1, whereas the effect due to the thermomagnetic torque is only as large as 1017, dyn cm−1.
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