HST and UKIRT imaging observations of z ∼ 1 6 C radio galaxies - I . The data
نویسنده
چکیده
The results of Hubble Space Telescope and UKIRT imaging observations are presented for a sample of 11 6C radio galaxies with redshifts 0.85 < z < 1.5. The observations of the 6C sources reveal a variety of different features, similar to those observed around the higher power 3CR sources of similar redshifts. However, the extent and luminosity of the aligned emission appears less extreme in the case of the 6C radio galaxies. For both samples, the aligned emission clearly cannot be explained by a single emission mechanism; line emission and related nebular continuum emission, however, often provide a significant contribution to the aligned emission.
منابع مشابه
High Redshift Css Radio Galaxies
We discuss CSS radio galaxies from 2 samples of radio sources. The rst sample is a complete sample of 28 3CR galaxies with redshifts in the range 0:6 < z < 1:8 for which we have HST, UKIRT and VLA imaging data. The 2 CSS galaxies contained in this sample, 3C49 and 3C241, appear to be less active than galaxies with radio sizes of order 50{100 kpc, but similar in activity to galaxies with radio s...
متن کاملHST and UKIRT imaging observations of z ∼ 1 6 C radio galaxies - II . Galaxy morphologies and the alignment effect
Powerful radio galaxies often display enhanced optical/UV emission regions, elongated and aligned with the radio jet axis. The aim of this series of papers is to separately investigate the effects of radio power and redshift on the alignment effect, together with other radio galaxy properties. In this second paper, we present a deeper analysis of the morphological properties of these systems, i...
متن کاملar X iv : a st ro - p h / 99 11 47 7 v 1 2 6 N ov 1 99 9 Galaxies at z > 5 : The View from Hawaii
We review the properties of z > 5 galaxies studied with HST and with the Keck telescopes, and discuss the detectability of Lyα emission-line galaxies out to z ∼ 6.5 based on these data and ongoing narrowband imaging surveys. The brightest sources may show (R − Z) color breaks, although the high sky background at Z (λeff ≈ 9200 Å), makes such observations challenging for typical faint sources. K...
متن کاملOPTICALLY FAINT COUNTERPARTS TO THE ISO-FIRBACK 170μm POPULATION: THE DISCOVERY OF COLD, LUMINOUS GALAXIES AT HIGH REDSHIFT
We present Keck spectroscopy and UKIRT near-IR imaging observations of two 170μm-selected sources from the ISO-FIRBACK survey which have faint counterparts in the optical, and r − K ∼ 5. Both sources were expected to lie at z > 1 based on their far-infrared, submillimeter and radio fluxes, assuming a similar spectral energy distribution to the local ultra-luminous infrared galaxy (ULIRG) Arp 22...
متن کاملLensing by Distant Clusters: Hst Observations of Weak Shear in the Field of 3c324
We present the detection of weak gravitational lensing in the eld of the radio galaxy 3C324 (z = 1:206) using deep HST imaging. From an analysis of the shapes of faint R = 24:5{27.5 galaxies in the eld we measure a weak, coherent distortion centered close to the radio source. This shear eld most likely arises from gravitational lensing of distant eld galaxies by a foreground mass concentration....
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
عنوان ژورنال:
دوره شماره
صفحات -
تاریخ انتشار 2003