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Characterizing the radio continuum emission from intense starburst galaxies [PDF]
Monthly Notices of the Royal Astronomical Society, 2016 The intrinsic thermal (free–free) and non-thermal (synchrotron) emission components that comprise the radio continuum of galaxies represent unique, dust-free measures of star formation rates (SFR). Such high SFR galaxies will dominate the deepest current
Timothy Galvin +2 more
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Detection of continuum radio emission associated with Geminga [PDF]
Monthly Notices of the Royal Astronomical Society: Letters, 2011 Abstract A deep Very Large Array observation of the Geminga pulsar field led to the discovery, at a higher than 10σ significance level, of radio emission trailing the neutron star proper motion. This ∼10 arcsec long radio feature, detected with a flux of ∼0.4 mJy at 4.8 GHz, is marginally displaced (2.7 ± 1.8 arcsec) from the pulsar ...
Andrea Possenti +2 more
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Spotless Flares and the Associated Radio Continuum Emission
Solar Physics, 1987.
Ruždjak, Vladimir +5 more
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Models of Uranian continuum radio emission
Journal of Geophysical Research: Space Physics, 1987The Uranian kilometric emissions detected by the Voyager 2 Planetary Radio Astronomy (PRA) experiment during the January 1986 encounter comprise two distinct types of emission: bursts and continuum. The bursts have been treated by Evans et al. (this issue). This paper considers the continuum emissions. The continuum emissions comprised four components:
Joseph H. Romig +4 more
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The ultraviolet continuum emission of radio galaxies
AIP Conference Proceedings, 1997This poster presents the UV continuum emission (in the range from 1400 to 3700 A) of radio galaxies (with redshift ranging from 0.01 to 0.1 and radio powers ranging from 1025 to 1027 Watts/Hz). The sample of radio galaxies were compiled by searching the Hubble Space Telescope (HST) archives for images taken with the Faint Object Camera (FOC) prior to ...
Esther L. Zirbel, Stefi A. Baum
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The infrared and radio-continuum emission of the galactic disk
Nature, 1987In 1983 the Infrared Astronomical Satellite (IRAS) surveyed the sky in four wavebands in the far infrared (FIR). One of the products of this survey1 is a detailed picture with an angular resolution of ∼4 arc min of the infrared emission of the interstellar dust in the galactic plane.
J L Osborne
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Radio continuum and CO emission in star-forming galaxies [PDF]
Astronomy and Astrophysics, 2002 We combine the radio continuum images from the NRAO VLA Sky Survey with the CO-line observations from the extragalactic CO survey of the Five College Radio Astronomy Observatory to study the relationship between molecular gas and the star formation rate within the disks of 180 spiral galaxies at 45" resolution. We find a tight correlation between these
Matteo Murgia +2 more
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Observations of the Solar Continuum Radio Emission at Decameter Wavelengths
AIP Conference Proceedings, 2010Results of study of the continuum radio emission of the Sun in the decameter range are presented. Observations were carried out with radio telescope URAN‐2 in summer months in 2008–2009. Radio fluxes at frequencies 20 MHz and 25 MHz in frequency band 250 kHz were obtained during the time, when there were no active regions on the solar disk.
Alexander Konovalenko +1 more
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Continuum radio emission from Virgo galaxies
Publications of the Astronomical Society of the Pacific, 1988The paper presents single-antenna measurements of radio emission from 120 galaxies in the Virgo cluster at 2380 MHz using a 2.6 arc min beam (half-power beam width). It also presents interferometric measurements at the same frequency for 48 galaxies with less than or equal to 1 arc sec resolution.
Kenneth C. Turner +2 more
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The radio continuum emission from the Galaxy
Symposium - International Astronomical Union, 1964Study of the radio continuum emission from the Galaxy is of interest both from the viewpoint of the physics of the radiating processes and the light which these shed on physical conditions within the Galaxy, and also because the large-scale organization of the emitting regions gives information about the structure of the Galaxy as a whole.
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