21.05.2014 Views

Radiation Transport Around Kerr Black Holes Jeremy David ...

Radiation Transport Around Kerr Black Holes Jeremy David ...

Radiation Transport Around Kerr Black Holes Jeremy David ...

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

136 CHAPTER 5. STEADY-STATE α-DISKS<br />

Figure 5-1: Comparison of hydrodynamic fluid variables for three versions of the<br />

steady-state α-disk model: Full numerical integration of the vertical structure equations<br />

(solid lines); The Novikov-Thorne approximation (dotted line); The revised<br />

analytic approximation derived in the text (dashed line). The black hole has mass<br />

M = 10M ⊙ , spin a/M = 0, and accretion rate Ṁ = 0.05 M ˙ Edd .

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!