STScI Preprint #1198

Dynamics and Excitation of Radio Galaxy Emission-Line Regions-I. PKS 2356-61

Results are presented from a programme of detailed longslit spectroscopic observations of the extended emission-line region (EELR) associated with the powerful radio galaxy PKS 2356-61. The observations have been used to construct spectroscopic datacubes, which yield detailed information on the spatial variations of emission-line ratios across the EELR, together with its kinematic structure. We present an extensive comparison between the data and results obtained from the MAPPINGS II shock ionization code, and show that the physical properties of the line-emitting gas, including its ionization, excitation, dynamics and overall energy budget, are entirely consistent with a scenario involving auto-ionizing shocks as the dominant ionization mechanism. This has the advantage of accounting for the observed EELR properties by means of a single physical process, thereby requiring less free parameters than the alternative scheme involving photoionization by radiation from the active nucleus. Finally, possible mechanisms of shock formation are considered in the context of the dynamics and origin of the gas, specifically scenarios involving infall or accretion of gas during an interaction between the host radio galaxy and a companion galaxy.

Status:

Appeared in: The Astrophysical Journal, 497:662-680, 1008

Affiliations:

¹) Space Telescope Science Institute 3700 San Martin Drive Baltimore, MD 21218 USA

²) ANU Astrophysical Theory Centre, Australian National University Canberra, ACT 0200, Australia³

³) The ANUATC is operated jointly by the Mount Stromlo and Siding Springs Observatories and the School of Mathematical Sciences of the Australian National University.