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A String of Radio Emission Associated with IRAS 16562-3959: A Collimated Jet Emanating from a Luminous Massive Young Stellar Object
(2010)
We report the discovery, made using the Australia Telescope Compact Array, of a remarkable string of radio emission toward IRAS 16562−3959, a luminous infrared source with a bolometric luminosity of 7.0×104 L . The radio ...
Probing the radio emission from air showers with polarization measurements
(American Physical Society - APSCollege Park, 2014-03)
The emission of radio waves from air showers has been attributed to the so-called geomagnetic emission process. At frequencies around 50 MHz this process leads to coherent radiation which can be observed with rather simple ...
Lateral distribution of the radio signal in extensive air showers measured with LOPES
(ElsevierAmsterdam, 2010)
The antenna array LOPES is set up at the location of the KASCADE-Grande extensive air shower experiment in Karlsruhe, Germany and aims to measure and investigate radio pulses from extensive air showers. The coincident ...
MHD numerical simulations of colliding winds in massive binary systems - I. Thermal versus non-thermal radio emission
(WILEY-BLACKWELLHOBOKEN, 2012)
In the past few decades detailed observations of radio and X-ray emission from massive binary systems revealed a whole new physics present in such systems. Both thermal and non-thermal components of this emission indicate ...
Synchrotron emission from secondary leptons in microquasar jets
(Springer, 2007)
Radio Variability in Seyfert Nuclei
(2009)
Comparison of 8.4-GHz radio images of a sample of 11 early-type Seyfert galaxies with previous observations reveals possible variation in the nuclear radio flux density in 5 of them over a 7-yr period. We find no correlation ...
Observed flux density enhancement at submillimeter wavelengths during an X-class flare
(Elsevier Sci LtdOxfordInglaterra, 2007)
Infrared-correlated 31-GHz radio emission from Orion East
(2010)
Lynds dark cloud LDN1622 represents one of the best examples of anomalous dust emission, possibly originating from small spinning dust grains. We present Cosmic Background Imager (CBI) 31 GHz data of LDN1621, a diffuse ...
A microwave study of coronal ejecta
(Univ Chicago PressChicagoEUA, 1999)