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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, ...

    D. F. De Mello, W. C. Keel, J. W. Sulentic, R. Rampazzo in Stellar Populations (1995)

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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...

    R. A. Windhorst, S. M. Pascarelle in Frontiers of Space And Ground-Based Astron… (1994)