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Chapter and Conference Paper
Stellar Populations in Mixed Pairs of Galaxies
The interpration of the interaction in galaxies is simplified in mixed pairs (E+S) because most or all of the cold gas can be traced to an origin in a single galaxy (S). We used spectroscopy, imaging, far-IR, ...
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Chapter
HST/FOS UV-Spectroscopy of Weak Radio Galaxies At z = 0.1-0.6
We present HSTFOS-spectra for 6 early-type weak radio galaxies with 0.08 < z < 0.53 and V = 17-21 mag. Most of these have deconvolved r -1/4 HST light-profiles out to z < 0.6. Lyman-α emission has...