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