Titlebook: Cooling Flows in Clusters and Galaxies; A. C. Fabian Book 1988 Kluwer Academic Publishers 1988 cosmic ray.cosmology.observatory.quasar.rel

玉米

t with the inflow rates predicted by X-ray data if the initial mass function resembles that in our Galaxy. It seems most likely that the bulk of the inflow in the clusters as well as in normal gE galaxies is deposited in the form of very low mass stars with 〈.〉 ? 0.7 M.. This efficient, low mass mod

Interim

sorbitol

bjectives are to search for extended blue continuum regions indicative of star formation, to study the spatial distribution of star formation, and to make a quantitative measure of the amount of light from young stars, which can lead to a measure of the star formation rate (for an assumed intial mas

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Die Verbreitung von Brustkrebs,or collimated ejection in PA 160 degrees. Outside this the radio structure bends rapidly by approximately 90 degrees before merging into the 10′ radio halo. It is suggested that the relativistic gas, which is responsible for the radio emission, may have a considerable effect on any cooling inflow ,

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Die Verbreitung von Brustkrebs,covering [OII]λ3727, H., [OIII] λ5007 and [SII]λλ6717, 6730 are presented. The line ratios are shown to be incompatible with the simplest model in which the gas is photoionized by a central active nucleus and lies at its projected distance from the nucleus.

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Ballerina

With the Westerbork Synthesis Radio Telescope (WSRT) we detect HI absorption at 5250 km/s in front of the nucleus of NGC 1275, with an optical depth of .003 and a dispersion of 205 km/s. We do not detect HI associated with the 30″ halo in absorption or emission.

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Eine Entwicklungsgeschichte der Brust,We show that the excitation of the filaments observed around NGC 1275 is more probably due to photoionization by the active nucleus radiation than to local radiative shocks. The photoionized gas is in pressure equilibrium with the hot ambient gas of the cooling flow.

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Characteristics of Extended Gas Around Radio Galaxies,A qualitative description is given of spectral properties, dynamical behaviour and morphology of a selection of mainly southern radio galaxies which have been observed to have extended ionized gas in their vicinity. The question of the significance of this gas in relation to cooling flows is still very much an open one.