Gas, dust, and star formation in distant radio galaxies Reuland, M.A.

Giant emission line halos surrounding distant radio galaxies provide unique lab- oratories for studying the feedback mechanisms that control the formation of massive

Emergence of cosmic structures around distant radio galaxies and quasars.. Overzier,

This has motivated an extensive program to study the properties of massive galaxy clusters in the early universe, using broad-band imaging with the HST/ACS Wide Field Channel (WFC),

(2001) suggested that high-redshift radio galax- ies and EROs could be identical galaxies seen at different stages of their evolution, based on their findings of ERO-like host

0156–252 is the only source in our sample for which the core is detected with sufficient S/N to carry out a (crude) spectral analysis. The X- ray spectrum is shown in Fig. The

Observations of cold dust in the submillimeter continuum, observations of CO lines ranging from probes of the cold (CO J=2–1 and 3–2), warm (CO J=6–5 and 7–6) , low density (C 18

Met de komst van hoge frequentie multi-pixel heterodyne instrumenten, zoals CHAMP + en HARP-B, zal het gebruik van spectraallijn-kaarten een veel centralere rol innemen in het

Using data taken with the Wide-Field Infrared Survey Explorer and Herschel Space Observatory physical properties of 6 dwarf elliptical galaxies (dEs) in the Fornax cluster and 19