Figure 3 from Modeling the Outflow in the Narrow-line Region of Markarian 573: Biconical Illumination of a Gaseous Disk

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Modeling the Outflow in the Narrow-line Region of Markarian 573: Biconical Illumination of a Gaseous Disk

Authors: T. C. Fischer, D. M. Crenshaw, S. B. Kraemer, H. R. Schmitt, and M. L. Trippe

FISCHER et al. 2010 The Astronomical Journal 140 577.

Provider: AAS Journals

Caption: Figure 3.

Kinematics model chosen as the best fit for our radial velocity data set. Parameters used to create this model are given in Table 1. Extended, lower velocity measurements outside 2'' from the nucleus are not enclosed in the model parameters as our model does not account for interactions with a disk.

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