arXiv · 0711.1164
Hypervelocity A & B Stars should be slow rotators
Abstract
The most commonly accepted explanation for the origin of hypervelocity stars in the halo of the Milky Way is that they are the result of tidal disruption of binaries by the massive black hole at the center of the Galaxy. We show that, if this scenario is correct, and if the original binary properties are similar to those in the local stellar neighbourhood, then the hypervelocity stars should rotate with velocities measureably lower than those for field stars of similar spectral type. This may prove to be a more direct test of the model than trying to predict the position and velocity distributions.
Explore related subjects
Keep this discovery
Brad Hansen. 2007-11-07. Hypervelocity A & B Stars should be slow rotators. https://doi.org/10.1086/525528
Cite the original work for its findings. Save a collection to share your selection of sources.