Understand
We present the combination of dynamical accretion model based on 3D GRMHD simulations and general relativistic (GR) polarized radiative transfer.
- We write down the formalism of and perform the GR ray-tracing of cyclo-synchrotron radiation through the model of accretion flow in Sagittarius A*.
- GR polarimetric imaging is presented as well as the results for spectrum for a probable set of spins and orientations.
- Precise fitting formulae for Faraday rotation and Faraday conversion coefficients are employed for thermal plasma.
Built on
Melrose, D. B. 1971 Ap&SS, 12, 172
1971
Earlier work this paper cites.
Melrose, D. B., McPhedran, R. C. 1991, ”Electromagnetic Processes in Dispersive Media”, (Cambridge University Press: Cambridge)
1991
Earlier work this paper cites.
Yuan, F., Quataert, E., Narayan, R. 2004, ApJ, 606, 894
2004
Earlier work this paper cites.
Similar
Macquart, J.-P., Bower, G. C., Wright, M. C. H., Backer, Donald C., Falcke, H. 2006, ApJ, 646, L111
2006
Cited alongside, same era.
Marrone, D. P., Moran, J. M., Zhao, J., & Rao R., 2007, ApJ, 654L, 57
2007
Cited alongside, same era.
Sharma, P., Quataert, E., Hammett, G. W., & Stone, J. M. 2007, ApJ, 667, 714
2007
Cited alongside, same era.
Then
Shcherbakov, R. V. 2008, ApJ, 688, 695
2008
Later among the works it cites.
Huang, L., Liu, S., Shen, Z.-Q., Yuan, Y.-F., Cai, M. J., Li, H., & Fryer, C. L. 2009, ApJ, 703, 557
2009
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