about
Ram pressure and dusty red galaxies – key factors in the evolution of the multiple cluster system Abell 901/902galapagos-c: analysis of galaxy morphologies using high-performance computing methodsThe host galaxies of X-ray selected active galactic nuclei to z = 2.5: Structure, star formation, and their relationships from CANDELS and Herschel/PACSMorphologies of z ∼ 0.7 AGN host galaxies in CANDELS: no trend of merger incidence with AGN luminosityThe impact from survey depth and resolution on the morphological classification of galaxiesIntegral field spectroscopy of nearby QSOs – I. ENLR size–luminosity relation, ongoing star formation and resolved gas-phase metallicities★
P2860
description
article publié dans la revue scientifique Astronomy and Astrophysics
@fr
im Dezember 2012 veröffentlichter wissenschaftlicher Artikel
@de
scientific article published in Astronomy and Astrophysics
@en
wetenschappelijk artikel
@nl
наукова стаття, опублікована в грудні 2012
@uk
name
AGN host galaxies at redshiftz ≈ 0.7: peculiar or not?
@en
AGN host galaxies at redshiftz ≈ 0.7: peculiar or not?
@nl
type
label
AGN host galaxies at redshiftz ≈ 0.7: peculiar or not?
@en
AGN host galaxies at redshiftz ≈ 0.7: peculiar or not?
@nl
prefLabel
AGN host galaxies at redshiftz ≈ 0.7: peculiar or not?
@en
AGN host galaxies at redshiftz ≈ 0.7: peculiar or not?
@nl
P2093
P2860
P356
P1476
AGN host galaxies at redshiftz ≈ 0.7: peculiar or not?
@en
P2093
A. N. Taylor
A. R. Robaina
C. Heymans
C. Y. Peng
D. H. McIntosh
E. F. Bell
E. van Kampen
P2860
P356
10.1051/0004-6361/201015444
P407
P577
2012-12-14T00:00:00Z
P818
P819
2013A&A...549A..46B