Almog Yalinewich
21.5.19
Star formation in extreme environments
Star - Central Black Hole interactions
Gas Accretion
Active
Very bright
Quiescent
very close
Tidal Radius
Apoapse Distance
To black hole
Tidal radius
gravitational radius
To black hole
black hole & accretion disc
cold outflow
cold ambient medium
hot outflow
hot ambient medium
Radio supernova
think about adiabatic compression
Accretion disc Jet
Accretion disc Jet
Unbound debris
Radio signal from ASASSN-14li
High impact parameter
Low impact parameter
high impact parameter
low impact parameter
Shocked region = 3 x obstacle size
Full loss cone
Empty loss cone
to the black hole
outside
Total number of stars
Stellar density slope
If there is no break
Governing equations can be solved analytically
Radio LoudĀ TDE -> density profile in a GC
Density profile -> Density of wind emitting stars
Wind emitting -> main sequence stars?
questions?