Star Formation in the Radio Galaxy NGC 4410A
Abstract
The NGC4410 group of galaxies provides us a rare opportunity to study a nearby (97 h75-1 Mpc) example of a radio galaxy (NGC4410A) embedded in an extended X-ray source, with evidence for star formation that can be readily spatially distinguished from regions dominated by the AGN and shocks. We present broadband and narrowband optical images along with optical and IUE ultraviolet spectroscopy for the radio galaxy NGC 4410A and its companion NGC 4410B. Our H-alpha+[NII] images reveal six luminous HII regions (LH-alpha ~ 1e40 erg/s distributed in an arc near NGC 4410A. Partially completing the ring is a prominent stellar loop containing diffuse ionized gas. This filamentary gas, in contrast to the H II regions, shows spectroscopic signatures of shock ionization. The star formation in this system may have been triggered by a collision or interaction between the two galaxies, perhaps by an expanding density wave, as in classical models of ring galaxies. Alternatively, the star formation may have been induced by the impact of a radio jet on the interstellar matter. Extended Ly-alpha is detected in the ultraviolet IUE spectrum. The ultraviolet continuum, which is presumably radiated by the nucleus of NGC4410A, is not extended. NGC4410A appears to be interacting with its neighbors in the NGC4410 group, and could be an example of a spiral galaxy transforming into an elliptical.
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