Cold Gas at High Redshift: Proceedings of a Workshop Celebrating the 25th Anniversary of the Westerbork Synthesis Radio Telescope, held in Hoogeveen, The Netherlands, August 28–30, 1995

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M.N. Bremer, P.P. van der Werf, H.J.A. Röttgering, C.L. Carilli
Springer Science & Business Media, Dec 6, 2012 - Science - 468 pages
Recent years have seen increasing evidence that the main epoch of galaxy formation in the universe may be directly accessible to observation. An gular fluctuations in the background relict radiation have been detected by various ground-based instruments as well as by the COBE satellite, and suggest that the epoch of galaxy formation was not so very early. Combined optical and radio studies have found galaxies at redshifts above 2. 0, systems that at least superficially show the characteristics expected of large galaxies seen only shortly after their formation. And absorption lines in the spectra of quasars seem to be telling us that most cold gas at early to intermediate cosmological epochs was in clouds having roughly galaxy sized masses. What kinds of new observations will best help us study this high redshift universe in future? What new instruments will be needed? These are questions that loom large in the minds of the Dutch astronom ical community as we celebrate 25 years of operation of the Westerbork Synthesis Radio Telescope. Celebration of this Silver Jubilee has included a birthday party (on 23 June, 1995), a commemorative volume looking at both the history and the future of the facility ("The Westerbork Observa tory, Continuing Adventure in Radio Astronomy," Kluwer 1996), and an international workshop, held in the village of Hoogeveen on 28-30 August, 1995.
 

Contents

CO in Ultraluminous and High z Galaxies 25
23
Dissipation in Forming Spheroidal
37
The Neutral Hydrogen Distribution in Luminous Infrared Galaxies 47
46
Molecular Gas and Dust in Infrared Luminous Galaxies
55
ELAIS
77
Hints to Galaxy Evolution
85
Small Scale Structure and High Redshift HI 93
92
H Weinberg L Hernquist N S Katz and J MiraldaEscudé
109
S Womble W L W Sargent and R S Lyons
254
cm Line Observations of Damped Lya Systems 267
279
Testing z 0 Analogs for the Damped Lyman a Absorbers
285
Molecular Gas in High Redshift Galaxies
293
and Possibly HCN in the Cloverleaf Quasar
301
Thermal Emission from Dust in Highz Galaxies 311
310
Submillimetre Observations of QSOs at Redshifts z 4
325
Radiative Transfer Models for IRAS F10214+4724 and other
337

On the Distribution of Intergalactic Clouds
115
Disk Galaxies at z 0 and at High Redshift
121
Warm Gas at High Redshift Clues to Gravitational Structure
137
HI Imaging of Clusters 145
144
An HI Survey of the Boötes Void
159
An HI Study of Ursa Major Spirals Dark Matter in Spirals
165
HI at High Redshift
171
ButcherOemler Effect and Radio Continuum 183
182
Warm Molecular Gas in AGNs and Cooling Flows
195
Xray Observations of Cold Gas in Clusters
205
Absorption Measurements of Molecular Gas
215
A New Molecular Absorption Line System The Gravitational
227
Deep HST Imaging of a Damped Lyman a Absorbing Galaxy
233
Associated Xray Absorption in High Redshift Quasars
239
Opacity of Singly Ionized Helium from Very Tenuous Intergalactic
245
a Hidden AGN?
343
Gas and Dust in high z radio galaxies
349
Kinematics and HI Absorption in Lyo Halos around z 2 Radio
363
The Effect of a Surrounding Cooling Flow on a Powerful Radio
373
N Bremer A C Fabian and C S Crawford
379
Dust and Obscuration
391
Radio Galaxies
397
HST Observations of Radio Galaxies at z 1
403
Studies of Cold Gas in the Early Universe with Large Millimeter
411
Strategies for Galaxy Surveys in the Submillimetre Waveband
423
Future Possibilities for Detecting HI at High Redshift
437
SPH Simulations of the Early Universe Performance of the Dwinge
451
Index
463
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