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Nuker Team : ウィキペディア英語版
Nuker Team
The Nuker Team was formed to use the Hubble Space Telescope, with its high-resolution imaging and spectroscopy, to investigate the central structure and dynamics of galaxies. The team used the HST to examine supermassive black holes and determined the relationship between a galaxy's central black hole's mass and velocity dispersion. The team continues to conduct research and publish papers on the supermassive black holes of galaxies and clusters.〔(Nuker Team Refereed Publications ).〕 The group was initially formed by Tod R. Lauer, then a first year postdoc. At the first meeting of the group held at Princeton University in June 1985, Sandra Faber was elected the group leader.
==Members==

The original members of the Nuker Team include Alan Dressler (OCIW), Sandra Faber (UCO/Lick; First PI), John Kormendy (Texas), Tod R. Lauer (NOAO), Douglas Richstone (Michigan; Present PI), and Scott Tremaine (IAS). Later additions to the team include Ralf Bender (Munchen), Alexei V. Filippenko (Berkeley), Karl Gebhardt (Texas), Richard Green (LBTO), Kayhan Gultekin (Michigan), Luis C. Ho (OCIW), John Magorrian (Oxford), Jason Pinkney (Ohio Northern), and Christos Siopis (Michigan).〔

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