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Gas Disks and Supermassive Black Holes in Nearby Radio Galaxies

Gas Disks and Supermassive Black Holes in Nearby Radio Galaxies

Gas Disks and Supermassive Black Holes in Nearby Radio Galaxies

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NGC 7052 (UGC 11718) This elliptical galaxy has a nuclear dust disk (b/a =<br />

0.30). It has a tw<strong>in</strong>-jet radio morphology on VLBA scales <strong>and</strong> a core-jet morphology<br />

on VLA scales. The STIS slits were aligned parallel to the galaxy major axis. The<br />

central k<strong>in</strong>ematic <strong>and</strong> flux properties are listed <strong>in</strong> Table 3.23; the gas exhibits a regular<br />

rotation profile. The fit to the central spectrum is not significantly improved by the<br />

addition of a broad component. Data for this galaxy are shown <strong>in</strong> Figure 3.20 (see<br />

key <strong>in</strong> Figure 3.1 for an explanation of these plots).<br />

UGC 12064 This S0 galaxy has a nuclear dust disk (b/a = 0.54). It has a tw<strong>in</strong>-jet<br />

radio morphology on VLA scales. The STIS slits were aligned parallel to the dust<br />

disk major axis. The central k<strong>in</strong>ematic <strong>and</strong> flux properties are listed <strong>in</strong> Table 3.24;<br />

the gas exhibits a regular rotation profile. The fit to the central spectrum is improved<br />

by the addition of a broad component. Data for this galaxy are shown <strong>in</strong> Figure 3.21<br />

(see key <strong>in</strong> Figure 3.1 for an explanation of these plots).<br />

NGC 7626 (UGC 12531) This elliptical peculiar galaxy has a nuclear dust lane<br />

(width : length = 0.17). It has a core-jet radio morphology on VLBA scales <strong>and</strong><br />

a tw<strong>in</strong>-jet morphology on VLA scales. The STIS slits were aligned parallel to the<br />

galaxy major axis. The central k<strong>in</strong>ematic <strong>and</strong> flux properties are listed <strong>in</strong> Table 3.25;<br />

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