1209.1104 (Gongjie Li et al.)
Gongjie Li, Abraham Loeb
We consider the long-term tidal heating of stars by the supermassive black hole at the Galactic center, SgrA*. We show that the accumulated heat deposited by excitation of stellar modes over many pericenter passages can lead to a runaway disruption of a star at a pericenter distance that is 7-10 times farther than the standard tidal disruption radius. The accumulated heating may explain the lack of massive ($\gtrsim 10M_{\odot}$) S-stars closer than several tens of AU from SgrA*.
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http://arxiv.org/abs/1209.1104
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