AGN: early BH suspicion Figure caption |
Accretion Disk and Jet Formation Figure caption |
Supernova, cataclismic Figure caption |
Supernova in NGC 4526 Figure caption |
Fading supernova light Figure caption |
SN 1987 in the LMC Figure caption |
SN remnants: Crab nebulae and Cassiopeia
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Kepler Supernova SN 1604 Figure caption |
Space-time curvature Figure caption |
The Helix nebula Figure caption |
Figure caption |
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The Dumbbell nebula Figure caption |
The Butterfly nebula Figure caption |
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M87 accretion gas disk Figure caption |
NGC 4261 with accretion disk Figure caption |
Star disruption near a BH Figure caption |
Black Holes grow by swallowing stars and gas. Their mass can become really large: 106 - 109 times the mass of the Sun (a few % of the parent galaxy mass). |
Gas dynamics Figure caption |
Stellar spectroscopy Figure caption |
< Stellar velocities Figure caption |
M32 - the advantage of high Figure caption |
Schwarzschild Method (my PhD thesis...) Figure caption |
The Galactic centre Figure caption |
Orbit of one star around Figure caption |
Orbiting stars near the Figure caption |
BH and Accretion disk appearance Figure caption |
Journey to a BH Credits |
background photo: Hubble Ultra Deep Field (Credit: NASA and ESA)
http://www.spacetelescope.org/news/html/heic0406.html