your ID: 0187 
First Name: Ye 
Last Name: Lu 
Affiliation: The national Astronomical Obsrvatoreis of China 

Title: The capture of a giant star or a main sequence star by
massive black holes
Authors: Y. Lu, Z. Zheng 
Topic: 1 
Session: oral 
Abstract: Since the mass-radius relation is quite different for a giant(G)
star and a main sequence (MS) star, we find that the radiation
efficiencies for the capture of a G star or a MS star are very
different. Given the mass of black holes, the results also show
that the size of the accretion disk formed by the tidal debris,
the involved viscose and the peak luminosity timescales for the
capture of G stars are larger than that for the capture of MS
stars. Paying special attention on the radiation efficiency of the
capture process, the radiation of the capture of a G star is
inefficiency, then relatively fainter, resulting in the total
energy of jets are relatively lower. All these may provide a
useful way to distinguish the capture of a G star from a MS star
star capture process.