Titlebook: Observational Cosmology; With the New Radio S M. N. Bremer,N. Jackson,I. Pérez-Fournon Conference proceedings 1998 Springer Science+Busines

歌剧等

HST Imaging of 3CR Radio Galaxies: The Dust-Radio Connectiontion between the radio source and the dust. The data cover a redshift range 0 < . < 0.5. A large range of dust morphologies is observed, including disk-like and filamentary structures..We find that there is a connection between the radio source and the dust. There is a strong tendency for the direct

横截,横断

洞察力

Slit-Lamp

NVSS Observations of UGC Galaxiese the NVSS limit of 2.5 mJy. Of particular note is that 41% of E and SO galaxies were detected. Approximately 25% of these have radio/IR flux density ratios consistent with star formation. Luminosity and visibility functions are derived for starforming and AGN powered radio sources. The normal galax

MIR

Radio-Optical Orientation of E/S0 Galaxies candidates were visually inspected on the Digitized Sky Survey (DSS) and on FIRST images: we find several spirals and interacting galaxies and a few E/S0s with very weak, marginally extended radio cores. The only double-lobed (previously known) radio source is a dumbbell. For the rest of the object

Blood-Vessels

A Wider View from the Southarkes and the University of Sydney Molonglo Observatory Synthesis Telescope (MOST). These will enable a number of large-scale surveys to be undertaken, complementing and in some cases surpassing what is being achieved in the North. This paper summarises the principal technical features of the new wi

BOOM

The Cambridge Low Frequency Radio Surveys: 6C, 7C, 8C of large areas of the northern sky at the very lowest available frequencies. The 7C survey—also at 151 MHz but with the higher resolution of 70 × 70cosecδ arcsec.—is currently being analysed and we now have catalogues in a number of selected regions, many of which have been observed repeatedly at a

hegemony

ADORE

Respond