搜索结果: 1-15 共查到“理学 Radio Continuum”相关记录16条 . 查询时间(0.093 秒)
Radio continuum observations of new radio halos and relics from the NVSS and WENSS surveys
Radio Continuum: galaxies – Galaxies: Clusters: general, intracluster medium – Cosmology: large-scale structure of Universe
2011/10/20
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...
Australia Telescope Compact Array radio continuum 1384 and 2368 MHz Observations of Sgr B
center synchrotron radiation cosmic rays molecular clouds general molecular clouds
2010/11/11
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 ...
Radio-continuum jets around the peculiar galaxy pair ESO 295-IG022
Galaxies clusters individual Abell S0102 – Galaxies individual
2010/11/10
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...
From pre- to young Planetary Nebulae: radio continuum variability
stars AGB and post-AGB circumstellar matter – radio continuum
2010/11/10
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...
Radio-continuum detections of Galactic Planetary Nebulae I. MASH PNe detected in large-scale radio surveys
Radio-continuum Galactic Planetary Nebulae I
2011/1/10
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
G34.26+0.15 G5.89-0.39 H92 Recombination Line
2009/6/11
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
Optical Molecular Outflows
2009/6/11
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 Emission KjPn 8 Planetary Nebula
2009/6/11
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
h i observations KJPN 8 remarkable planetary nebula
2009/6/11
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
Radio Continuum Planetary Nebulae
2009/6/4
Radio Continuum and H I Observations of the Remarkable Planetary Nebula KJPN 8
Radio Continuum and Far-infrared Emission from the Galaxies in the Eridanus Group
radio continuum radio–FIR correlation galaxies
2009/5/12
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...
A RADIO-CONTINUUM STUDY OF THE SUPERNOVA REMNANT MSH 11-61A
ISM individual objects (MSH 11-61A, G290.1-0.8)-ISM supernova remnants-radio continuum ISM
2009/2/26
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 ...
RADIO CONTINUUM STUDY OF THE LARGE MAGELLANIC CLOUD - SNR J0519-6926
ISM supernova remnants-Magellanic Clouds-ISM individual ob-jects SNR J0519-6926
2009/2/9
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...