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The Central Kiloparsec of Seyfert and Inactive Host Galaxies: a Comparison of Two-Dimensional Stellar and Gaseous Kinematics.

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Academic year: 2021

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Figure

Figure 1. R-band Digital Sky Survey images of the sample galaxies. The ’(S)’ or ’(C)’ on the right of the object names stand for Seyfert or Control galaxy, respectively
Table 1. Properties of our sample. (1) Pairs identifier, (2) Galaxy name, (3) Hubble Type (NED), (4) Numerical morphological type (LEDA), (5) Distance in Mpc (Ho et al
Table 2. Details of the exposures of our sample. (1) Pairs identi- identi-fier, (2) NGC number, (3) date of observation (4) Exposure time in sec, (5) Seeing, Full Width at Half Maximum in arcseconds.
Figure 2. Examples of spectra and their corresponding fits for 4 galaxies. (a): NGC 2985 (inactive), (b): NGC 3227 (Seyfert 1.5), (c):
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