Results 271 to 280 of about 84,001 (296)
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Radio Continuum Emission from Galaxies

1975
The continuum radio emission detected from external galaxies is produced either by thermal process or by the synchrotron process with the latter dominating in most cases. For the synchrotron process the volume emissivity is given by $$ \varepsilon \left( \upsilon \right) = {\rm{n}}{\mkern 1mu} {{\rm{B}}^{\frac{{{\rm{1 + }}\gamma }}{2}}} {\upsilon ^{
openaire   +1 more source

Radio Continuum and CO emission in spiral galaxies

2023
We have studied the relationship between the Radio Continuum (RC) and CO emission for a set of galaxies selected from the BIMA SONG sample. By combining new 20 cm VLA B-array observations with BIMA maps it has been possible to investigate the behaviour of the RC/CO correlation at matched resolution down to an angular size of about 6''.
Paladino, Rosita   +7 more
openaire   +1 more source

Splotless flares and the associted radio continuum emission

Solar physics, 1987
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Ruždjak, Vladimir, Vršnak, Bojan
openaire  

Water Masers and Radio Continuum Emission Tracing Thermal Radio Jets

2009
We present interferometric observations of radio continuum and water maser emission carried out with the Very Large Array (VLA1) toward five massive star-forming regions. Radio continuum sources were detected toward all star-forming regions and some of them could be thermal radio jets. In addition, although water maser emission was found in all massive
openaire   +1 more source

The tiered radio extragalactic continuum (T-RECS) simulation II: H i emission and continuum-H i cross-correlation

Monthly Notices of the Royal Astronomical Society, 2023
Anna Bonaldi, G De Zotti, M Bonato
exaly  

Evolution of thermal and non-thermal radio continuum emission on kpc scales – predictions for SKA

Monthly Notices of the Royal Astronomical Society, 2022
M Ghasemi-Nodehi   +2 more
exaly  

The Large-Scale Radio Continuum Emission of Spiral Galaxies

1990
In this paper I review the recent results on the radio continuum emission from spiral galaxies. The emphasize is on the large-scale non-thermal emission which arises from the interaction between cosmic ray electrons and magnetic fields.
openaire   +1 more source

Studies of ultracompact H ii regions - II. High-resolution radio continuum and methanol maser survey

Monthly Notices of the Royal Astronomical Society, 1998
A J Walsh, M G Burton, A R Hyland
exaly   +2 more sources

Characterizing the radio continuum emission from intense starburst galaxies

Monthly Notices of the Royal Astronomical Society, 2016
T J Galvin, N Seymour, M D Filipovic
exaly  

Anisotropic Optical Continuum Emission in Radio Quasars

1994
J. C. Baker   +3 more
openaire   +1 more source

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