✦ LIBER ✦

Evolutionary models of powerful radio galaxies

✍ Scribed by G. V. Bicknell; R. S. Sutherland

Publisher: John Wiley and Sons
Year: 2006
Tongue: English
Weight: 305 KB
Volume: 327
Category: Article
ISSN: 0004-6337
DOI: 10.1002/asna.200510514

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

The lifecycles of powerful radio galaxie

The lifecycles of powerful radio galaxies: Triggering and feedback

✍ C. Tadhunter 📂 Article 📅 2006 🏛 John Wiley and Sons 🌐 English ⚖ 211 KB 👁 2 views

## Abstract I review the links between host galaxy evolution and quasar/jet activity in radio galaxies from an observational standpoint. Observations of the warm ionized gas provide evidence for powerful outflows in both the extended emission line regions (EELR: 5 < __r__ < 100 kpc) and the narrow

Evolution of radio galaxies

✍ C.R. Kaiser 📂 Article 📅 2009 🏛 John Wiley and Sons 🌐 English ⚖ 121 KB 👁 2 views

Radio emission of galaxy clusters

✍ I. Golombek; M. Bartelmann; T. Enßlin; M. Jubelgas; C. Pfrommer; V. Springel 📂 Article 📅 2006 🏛 John Wiley and Sons 🌐 English ⚖ 204 KB 👁 2 views

Radio spectra of some markarian galaxies

✍ D. F. Dickinson; G. Kojoyan; C. R. Purton; R. A. Sramek; H. M. Tovmassian 📂 Article 📅 1976 🏛 John Wiley and Sons 🌐 English ⚖ 176 KB 👁 1 views

The radio luminosity function of radio g

The radio luminosity function of radio galaxies in distant clusters

✍ M. Branchesi; I. M. Gioia; C. Fanti; R. Fanti; R. Perley 📂 Article 📅 2006 🏛 John Wiley and Sons 🌐 English ⚖ 72 KB 👁 2 views

## Abstract A complete sample of 18 X‐ray selected clusters of galaxies belonging to the __ROSAT__ North Ecliptic Pole (NEP) survey has been observed with the Very Large Array at 1.4 GHz. These are the most distant clusters in the X‐ray survey with redshift in the range 0.3 < __z__ < 0.8. 79 radio

On the question of radio emission of spi

On the question of radio emission of spiral galaxies in groups of galaxies

✍ V. H. Malumian 📂 Article 📅 1996 🏛 John Wiley and Sons 🌐 English ⚖ 423 KB 👁 1 views

It has been shown that the radio emission properties of spiral galaxies, if the other conditions are the same, are determined rather by the presence of the close neighbours than by space density of galaxies around them. The rate of occurence of radio sources and their radio luminosities among the sp