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The evolution of active galaxies in cluster environments

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The evolution of active galaxies in cluster environments Powered By Docstoc
					Binding energies of different elements
Helium-burning
AGB stars
Heavier element burning
Electron degeneracy
Neutron star structure
Neutron
 star
masses
Detecting
 black
 holes
Optical and radio
studies provide
evidence for black
holes at centres of
galaxies: 106-109
solar masses within
0.5 light years
Stellar motions in the Galactic Centre
Stellar motions in the galactic centre

				
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