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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, Osborne J L
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Decimeter continuum radio emission from a post-flare loop
Solar Physics, 1986Radio observations offer an important means for providing estimates of magnetic fields in post-flare loops.
M R Kundu, Kundu M R
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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.
A A Konovalenko, V V Dorovskyy
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Properties of the Radio Continuum Emission from Interacting Galaxies
Nature, 1973SEVERAL interacting galaxies have been observed recently in different programmes using the Westerbork Synthesis Radio Telescope at 21 cm wavelength (beamwidth 24 s × 24 s cosec δ). We give here a compilation of the data in order to examine the morphology, strength, and the frequency of occurrence of the radio emission from these interacting systems.
R J Allen, R D Ekers, G K Miley
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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
T J Galvin, N Seymour, M D Filipovic
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Monthly Notices of the Royal Astronomical Society, 2023 In this paper we extend the Tiered Radio Extragalactic Continuum Simulation (T-RECS) to include HI emission. The HI T-RECS model is based on the most recent HI mass function estimates, combined with prescriptions to convert HI mass to total integrated HI
Anna Bonaldi, G De Zotti, M Bonato
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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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