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搜索结果: 1-15 共查到理学 Radio-continuum相关记录16条 . 查询时间(0.109 秒)
Radio halos and relics are diffuse radio sources found in galaxy clusters showing significant substructure at X-ray wavelengths. These sources provide important information about non-thermal processes...
We present images of the Sagittarius (Sgr) B giant molecular cloud at 2368 and 1384 MHz obtained using new, multi-configuration Australia Telescope Compact Array (ATCA) observations. We have combined ...
We report new radio-continuum observations with the Australia Telescope Compact Array (ATCA) of the region surrounding the peculiar galaxy pair ESO295-IG022, at the centre of the poor cluster Abell S0...
Searching for variability, we have observed a sample of hot post-AGB stars and young Planetary Nebulae candidates with the Very Large Array at 4.8, 8.4, and 22.4 GHz.The sources had been previously de...
We present an updated and newly compiled radio-continuum data-base for MASH PNe detected in the extant large scale "blind" radio-continuum surveys (NVSS, SUMSS/MGPS-2 and PMN) and, for a small number ...
Radio continuum sources associated with AB Aur。
Radio Continuum and H92 Recombination Line Observations of G34.26+0.15 and G5.89-0.39。
Radio Continuum Observations towards Optical and Molecular Outflows。
Time Variation in the Radio Continuum Emission Associated with the Surroundings of the Nucleus of the Planetary Nebula KjPn 8。
Radio continuum and h i observations of the remarkable planetary nebula KJPN 8
VLA radio continuum observations of WR ring nebulae。
Radio Continuum and H I Observations of the Remarkable Planetary Nebula KJPN 8
The Eridanus galaxies follow the well-known radio–FIR correlation. The majority (70%) of these galaxies have their star formation rates below that of the Milky Way. The galaxies that have a signific...
We present a high-resolution radio-continuum study of Galactic supernova remnant MSH11{61A. We combine moderate resolution X-ray, radio- continuum and CO data to study the morphology and kinematics ...
We present the results of new high resolution ATCA observations of SNR J0519{6926. We found that this SNR exhibits a typical "horseshoe" ap- pearance with ®={0.55§0.08 and D=28§1 pc. No polariza...

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