6 April 2006
6 April 2006
Speaker: Warren Brown (CfA)
Title:
Clay Fellowship Lecture:
Hypervelocity Stars Ejected from the Galactic Center
Abstract:
A natural consequence of a massive black hole in a dense stellar
environment like the Galactic Center is the creation of "hypervelocity
stars," stars ejected at extreme velocities from the Galaxy. Last year we
announced the discovery of the first hypervelocity star: a 3 solar mass
main sequence B star, just like the stars seen in the Galactic Center, but
at a distance 110 kpc from the Galactic Center. We have designed a
successful targeted survey for new hypervelocity stars, and discuss our
newest discoveries. Because hypervelocity stars originate from a close
encounter with a massive black hole, hypervelocity stars can be used as
important tools for understanding the nature and environs of black holes.
Our recent discoveries allows us to place interesting limits on the mass
function of stars in the Galactic center and the history of stellar
interactions with the massive back hole.
Video of the Presentation
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