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Program Number |
161 |
| Program Name | FRI/FRII Radio Galaxy Morphology Dichotomy |
| Principal Investigator |
Hermine Landt [email] [web] |
| Co-Investigator(s) | |
Abstract |
We propose to obtain at the MMT stellar velocity dispersion measurements for 19 radio galaxies and at the FLWO 1.5 m narrow emission line fluxes for 16/19 sources in order to derive their black hole masses and accretion rates. These observations will allow us to test the recent claim that the FR I/FR II radio morphology dichotomy for radio galaxies can be mainly attributed to a change in accretion mode. The result will be a deeper understanding of the jet-accretion disk connection and the jet production mechanism in active galactic nuclei (AGN). |
| Spectra | [search in archive] |
| Trimester(s) data taken | 2005b |
| Papers | none |
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