Detection of a large mass of dust in a radio galaxy at redshift z = 3.8
Authors:
- 1 August 1994
- journal article
- letter
- Published by Springer Nature in Nature
- Vol. 370 (6488) , 347-349
Abstract
No abstract availableKeywords
This publication has 24 references indexed in Scilit:
- Radio continuum polarimetric imaging of high redshift radio galaxiesThe Astronomical Journal, 1994
- Luminosity dependence of optical activity and alignments into radio galaxiesMonthly Notices of the Royal Astronomical Society, 1993
- Infrared spectroscopy of 11 radio galaxies at Z equals 2-4 - Evidence that some high-redshift radio galaxies may be protogalaxiesThe Astrophysical Journal, 1993
- Evidence that the z = 3.4 radio galaxy B2 0902+34 may be a protogalaxyNature, 1993
- A search for primeval galaxies using a narrow-band imaging techniqueThe Astronomical Journal, 1993
- Hubble Space Telescope imaging of distant galaxies - 4C 41.17 at Z = 3.8The Astrophysical Journal, 1992
- The optical polarizations of high- and intermediate-redshift radio galaxiesMonthly Notices of the Royal Astronomical Society, 1992
- 4C 41.17 - A radio galaxy at a redshift of 3.8The Astrophysical Journal, 1990
- An infrared search for primeval galaxiesMonthly Notices of the Royal Astronomical Society, 1988
- The smoothness of the 2.2 micron background - Constraints on models of primeval galaxiesThe Astrophysical Journal, 1986