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Radiation Transfer of Emission Lines in Curved Space-Time

Steven V. Fuerst·Kinwah Wu
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Abstract

We present a general formulation for ray-tracing calculations in curved space-time. The formulation takes full account of relativistic effects in the photon transport and the relative motions of the emitters and the light-of-sight absorbing material. We apply the formulation to calculate the emission from accretion disks and tori around rotating black holes.

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Steven V. Fuerst, Kinwah Wu. 2004-06-17. Radiation Transfer of Emission Lines in Curved Space-Time. https://doi.org/10.1051/0004-6361%3A20035814

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