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Time-evolution of ionization and heating around first stars and miniqsos
Rajat M. Thomas,
Saleem Zaroubi
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Keyphrases
Temperature Profile
100%
First Stars
100%
Heating Pattern
100%
Population III Stars
100%
Black Men
50%
Switch-off
50%
Radio
50%
Radio Telescope
50%
High Energy Photons
50%
X-ray
50%
Spectral Shape
50%
Intergalactic Medium
50%
Medium Temperature
50%
Radiative Transfer
50%
Helium
50%
LOFAR
50%
Brightness Temperature
50%
Radiative Transfer Code
50%
Radiative Transfer Calculation
50%
Analytical Approach
50%
Inappropriate Treatment
50%
Analytical Approximation
50%
Secondary Collision
50%
Outer Radius
50%
Physics
Population III Stars
100%
Radiative Transfer
75%
Temperature Profile
50%
Radio Telescope
25%
Intergalactic Medium
25%
LOFAR
25%
Brightness Temperature
25%