Rotation of the protostar helps generate the magnetic fields and bipolar flows.

True
False

Since this is not my area of expertise, I searched Google under the key words "protostar rotation magnetic" to get these possible sources:

http://www.aas.org/publications/baas/v33n4/aas199/83.htm
http://www.astro.psu.edu/users/edf/araa/node9.html
http://adsabs.harvard.edu/abs/2001AAS...199.3705B
http://72.14.253.104/search?q=cache:OVTq6LKaslIJ:www.lpi.usra.edu/meetings/ppv2005/pdf/8580.pdf+protostar+rotation+magnetic&hl=en&gl=us&ct=clnk&cd=10&client=safari
(Broken Link Removed)
http://www.aoc.nrao.edu/~smyers/courses/astro12/L14.html

I hope this helps. Thanks for asking.

True

The statement "Rotation of the protostar helps generate the magnetic fields and bipolar flows" is true. During the formation of a protostar, as the cloud of gas and dust collapses under its own gravity, it starts to spin due to the conservation of angular momentum. This rotation plays a crucial role in the generation of magnetic fields and the formation of bipolar flows.

To understand this further, you can refer to the sources provided in the Google search results. The sources will provide more detailed information about the processes involved in the generation of magnetic fields and bipolar flows in protostars.

- The first source (http://www.aas.org/publications/baas/v33n4/aas199/83.htm) appears to be a conference abstract that discusses the magnetic fields and outflow properties in protostars.

- The second source (http://www.astro.psu.edu/users/edf/araa/node9.html) is an article from the Annual Review of Astronomy and Astrophysics. It provides a comprehensive review of protostellar disks, including their rotation and the generation of magnetic fields.

- The third source (http://adsabs.harvard.edu/abs/2001AAS...199.3705B) seems to be a conference poster that discusses the observations of magnetic fields in protostars.

- The fourth source is a broken link to a PDF file.

- The fifth source (http://www.aoc.nrao.edu/~smyers/courses/astro12/L14.html) is a lecture note that covers various topics related to protostars, including the role of rotation in the formation of magnetic fields and outflows.

By referring to these sources, you can gain a deeper understanding of how rotation influences the generation of magnetic fields and bipolar flows in protostars.