玉米
发表于 2025-3-23 10:12:49
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
发表于 2025-3-23 14:56:18
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sorbitol
发表于 2025-3-23 18:09:21
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
体贴
发表于 2025-3-24 01:55:29
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提名的名单
发表于 2025-3-24 03:33:23
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 ,
要控制
发表于 2025-3-24 07:56:30
Die Verbreitung von Brustkrebs,covering λ3727, H., λ5007 and 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.
口味
发表于 2025-3-24 11:54:57
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Ballerina
发表于 2025-3-24 18:45:55
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.
狼群
发表于 2025-3-24 22:49:26
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.
过于平凡
发表于 2025-3-25 02:25:12
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.