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11.13. Gravitational waves generated by globular cluster systems collapse

Published online by Cambridge University Press:  25 May 2016

R. Capuzzo-Dolcetta  and
P. Miocchi
R. Capuzzo-Dolcetta
Affiliation:
Istituto Astronomico (Univ. of Rome “La Sapienza”) via G.M. Lancisi 29, I-00161 - Rome, Italy
P. Miocchi
Affiliation:
Dep. of Physics (Univ. of Rome “La Sapienza”) P.le Aldo Moro 5, I-00185 - Rome, Italy

Extract

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The hypothesis -raised and discussed in - that the source of AGN fueling can be, at least in elliptical galaxies, stars belonging to a dense stellar environment formed by globular clusters frictionally decayed and tidally destroyed by the gravitational field of central black hole (b.h.), is strongly supported in. The quantity of star mass swallowed by the b.h. and its time rate seem at all compatible with those needed to justify the intensity and time characteristics of galactic nuclei activity (see also).

Type
Part III. Black Holes and Central Activity
Information
Symposium - International Astronomical Union , Volume 184: The Central Regions of the Galaxy and Galaxies , 1998 , pp. 481 - 482
Copyright
Copyright © Kluwer 1998 

References

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