BRIGHT lights, BIG city: Massive galaxies, giant Ly-a nebulae, and proto--clusters
arXiv:astro-ph/0209173
Abstract
High redshift radio galaxies are great cosmological tools for pinpointing the most massive objects in the early Universe: massive forming galaxies, active super--massive black holes and proto--clusters. We report on deep narrow--band imaging and spectroscopic observations of several z > 2 radio galaxy fields to investigate the nature of giant Ly-alpha nebulae centered on the galaxies and to search for over--dense regions around them. We discuss the possible implications for our understanding of the formation and evolution of massive galaxies and galaxy clusters.
arXiv commentPaper presented at the SPIE conference on Astronomical Telescopes and Instrumentation `Discoveries and Research Prospects from 6 - 10m Class Telescopes II', August 22, 2002, Waikoloa, Hawaii USA
References in corpus (16)
- The Demography of Massive Dark Objects in Galaxy Centres
- Mass function of dark matter halos
- Cooling Radiation and the Lyman-alpha Luminosity of Forming Galaxies
- A submillimetre survey of the star-formation history of radio galaxies
- Triggered Star Formation in a Massive Galaxy at z=3.8: 4C41.17
- Jet-Induced Emission-Line Nebulosity and Star Formation in the High-Redshift Radio Galaxy 4C41.17
- Interaction of Radio Lobes with the Hot Intracluster Medium: Driving Convective Outflow in Hydra A
- An IR-Selected Galaxy Cluster at z=1.27
- Buoyant radio plasma in clusters of galaxies
- CO emission and associated HI absorption from a massive gas reservoir surrounding the z=3 radio galaxy B3 J2330+3927
- A Pair of Compact Red Galaxies at Redshift 2.38, Immersed in a 100 kpc Scale Ly-alpha Nebula
- A Tunable Lyot Filter at Prime Focus: a Method for Tracing Supercluster Scales at z ~ 1
- A search for clusters at high redshift - II. A proto cluster around a radio galaxy at z=2.16
- HST images and properties of the most distant radio galaxies
- A vestige low metallicity gas shell surrounding the radio galaxy 0943-242 at z=2.92
- LIFTS: an Imaging Fourier Transform Spectrograph for Astronomy