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- W4293232159 abstract "Aims. The only relativistic reflection model that implements a parameter relating the intensity incident on an accretion disk to the observed intensity is relxill. The parameter used in earlier versions of this model, referred to as the reflection strength, is unsatisfactory; it has been superseded by a parameter that provides insight into the accretion geometry, namely the reflection fraction. The reflection fraction is defined as the ratio of the coronal intensity illuminating the disk to the coronal intensity that reaches the observer." @default.
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- W4293232159 date "2016-05-13" @default.
- W4293232159 modified "2023-10-18" @default.
- W4293232159 title "Normalizing a relativistic model of X-ray reflection" @default.
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- W4293232159 doi "https://doi.org/10.1051/0004-6361/201628135" @default.
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