VLT spectropolarimetry of two powerful radio galaxies at z ∼ 1.4: Ultraviolet continuum, emission-line properties and the nature of high-redshift dust

Monthly Notices of the Royal Astronomical Society

Volumn 351, Issue 3, 2004, Pages 997-1014

  Solorzano Inarrea C ^a   Best, P N ^a   Rottgering H J A ^b   Cimatti, A ^c  

^a UNIVERSITY OF EDINBURGH   (United Kingdom)

^b LEIDEN UNIVERSITY   (Netherlands)

^c Istituto Nationale di Astrofisica   (Italy)

Author keywords

Galaxies: active; Galaxies: evolution; Galaxies: ISM; Polarization; Radio continuum: galaxies; Scattering

Indexed keywords

COSMOLOGY; DUST; ELECTROMAGNETIC WAVE EMISSION; GALAXIES; PHOTOIONIZATION; RADIO ASTRONOMY;

CONTINUUM EMISSION; EMISSION LINES; FLUX SPECTRUM; GALAXIES ACTIVE; GALAXIES: ISM; GALAXY EVOLUTION; PROPERTY; RADIO CONTINUUM: GALAXIES; RADIO GALAXIES; WAVELENGTH RANGES;

POLARIZATION;

EID: 3042858911     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.07842.x     Document Type: Article

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