Figure 14 from Submillimeter Array/Plateau de Bure Interferometer Multiple Line Observations of the Nearby Seyfert 2 Galaxy NGC 1068: Shock-related Gas Kinematics and Heating in the Central 100 pc?

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Submillimeter Array/Plateau de Bure Interferometer Multiple Line Observations of the Nearby Seyfert 2 Galaxy NGC 1068: Shock-related Gas Kinematics and Heating in the Central 100 pc?

Authors: M. Krips, S. Martín, A. Eckart, R. Neri, S. García-Burillo, S. Matsushita, A. Peck, I. Stoklasová, G. Petitpas, A. Usero, F. Combes, E. Schinnerer, L. Humphreys, and A. J. Baker

Krips et al. 2011 The Astrophysical Journal 736 37.

Provider: AAS Journals

Caption: Figure 14.

Spatially averaged line ratio for the eastern and western knots as a function of velocity, derived from Figure 13. The error bars denote the variance of each averaged value, which does not exceed 50% in most cases. The missing values for velocities of −120 and −200 km s ⁻¹ and +100 to +140 km s ⁻¹ are due to the lack of emission in the respective knot. The dashed lines represent the median of the line ratios for the two knots.

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