Alignment of Protostars and Circumstellar Disks during the Embedded Phase
Abstract
Star formation proceeds via the collapse of a molecular cloud core over multiple dynamical timescales. Turbulence within cores results in a spatially non-uniform angular momentum of the cloud, causing a stochastic variation in the orientation of the disk forming from the collapsing material. In the absence of star–disk angular momentum coupling, such disk-tilting would provide a natural mechanism for the production of primordial spin–orbit misalignments in the resulting planetary systems. However, owing to high accretion rates in the embedded phase of star formation, the inner edge of the circumstellar disk extends down to the stellar surface, resulting in efficient gravitational and accretional angular momentum transfer between the star and the disk. Here, we demonstrate that the resulting gravitational coupling is sufficient to suppress any significant star–disk misalignment, with accretion playing a secondary role. The joint tilting of the star–disk system leads to a stochastic wandering of star-aligned bipolar outflows. Such wandering widens the effective opening angle of stellar outflows, allowing for more efficient clearing of the remainder of the protostar's gaseous envelope. Accordingly, the processes described in this work provide an additional mechanism responsible for sculpting the stellar initial mass function.
Additional Information
© 2014 The American Astronomical Society. Received 29 October 2014, accepted for publication 19 November 2014; Published 9 December 2014. We thank Richard Nelson for useful discussions and the Michigan Institute for Research in Astrophysics for helping to facilitate this collaboration.Attached Files
Published - 2041-8205_797_2_L29.pdf
Submitted - 1411.5431v2.pdf
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Additional details
- Eprint ID
- 54418
- Resolver ID
- CaltechAUTHORS:20150205-103518121
- Created
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2015-02-05Created from EPrint's datestamp field
- Updated
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2021-11-10Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences