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The VLA Survey of the Chandra Deep Field South. V. Evolution and Luminosity Functions of sub-mJy radio sources and the issue of radio emission in radio-quiet AGN
Chandra Deep Field Luminosity Functions radio sources radio emission
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2011/10/9
We present the evolutionary properties and luminosity functions of the radio sources belonging to the Chandra Deep Field South VLA survey, which reaches a flux density limit at 1.4 GHz of 43 microJy a...
The Evolution of Radio Galaxies and X-ray Point Sources in Coma Cluster Progenitors Since z~1.2
Evolution Radio Galaxies Point Sources Cluster Progenitors Since
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2011/9/30
Using Chandra imaging spectroscopy and Very Large Array (VLA) L-band radio maps, we have identified radio sources at P_{1.4GHz} >=5x10^{23} W Hz^{-1} and X-ray point sources (XPSs) at L_{0.3-8keV}>=5x...
Radio emission models of Colliding-Wind Binaries
Radio emission models Colliding-Wind Binaries
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2009/6/15
Radio emission models of Colliding-Wind Binaries。
Biodiversity loss in the orion radio zoo?
Radio Continuum and Far-infrared Emission from the Galaxies in the Eridanus Group
radio continuum radio–FIR correlation galaxies
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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...
THE RELATION BETWEEN RADIO FLUX DENSITY AND IONISING ULTRA-VIOLET FLUX FOR HII REGIONS AND SUPERNOVA REMNANTS IN THE LARGE MAGELLANIC CLOUD
Galaxies Magellanic Clouds-ISM HII regions-ISM supernova remnants-radio continuum galaxies-ultraviolet galaxies
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2009/3/12
We present a comparison between the Parkes radio surveys (Filipovi
´c et al. 1995) and Vacuum Ultra-Violet (VUV) surveys (Smith et al. 1987)
of the Large Magellanic Clouds (LMC). We have found...