Results 1 to 10 of about 267 (136)
INTEGRATED RADIO CONTINUUM SPECTRA OF GALAXIES [PDF]
The Astronomical Journal, 2015 13 pages, 13 figures, 5 tables; accepted for publication in the Astronomical ...
Marvil, Joshua +2 more
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Radio Continuum Imaging of High‐Redshift Radio Galaxies [PDF]
The Astrophysical Journal Supplement Series, 1997 ApJ (Supplement) (paper no. 33814)
Carilli, C. L. +4 more
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Radio continuum morphology of southern Seyfert galaxies [PDF]
Astronomy and Astrophysics Supplement Series, 1999 We present radio observations for 29 southern Seyfert galaxies selected from a volume limited sample with cz<3600 km s^-1, and declination delta<0degr.
Morganti, R. +3 more
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Radio continuum properties of luminous infrared galaxies [PDF]
Astronomy & Astrophysics, 2015 33 pages, 7 figures, 5 tables, to appear in A& ...
Vardoulaki, E. +9 more
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Radio continuum properties of OH megamaser galaxies [PDF]
Monthly Notices of the Royal Astronomical Society, 2021 ABSTRACT We present a study of the radio continuum properties of two luminous/ultraluminous infrared galaxy samples: the OH megamaser (OHM) sample (74 objects) and the control sample (128 objects) without detected maser emission. We carried out pilot observations for 140 objects with the radio telescope RATAN-600 at 1.2, 2.3, 4.7, 8.2 ...
Yu V Sotnikova +14 more
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Radio Continuum Surveys of the Galaxy and Galaxies [PDF]
Symposium - International Astronomical Union, 2002 Radio sky surveys give us basic information about the origin of the radio emission from the Galaxy. By mapping the sky at several radio frequencies a separation of the thermal and non-thermal emission components is possible. The major part of the low-frequency radio emission comes from the synchrotron process, the braking of relativistic electrons in ...
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Radio Continuum Emission in Polar Ring Galaxies
The Astronomical Journal, 2004 We have used the Very Large Array aperture synthesis telescope to conduct a radio continuum survey of polar-ring galaxies, at 20cm and 6cm. Forty objects were observed at 20cm with 5" resolution. Twenty (50%) of the program sources were detected at 20cm, down to our 5-sigma limit of 0.5 mJy/beam.
Cox, A. L., Sparke, L. S.
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The molecular connection to the FIR-radio continuum correlation in galaxies [PDF]
Astronomy & Astrophysics, 2005 Accepted by A&A, 25 pages, 10 figures.
Murgia, M. +6 more
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Radio continuum emission of the Milky Way and nearby galaxies [PDF]
Symposium - International Astronomical Union, 1985 The radio continuum emission of the Milky Way and nearby galaxies can be decomposed into a central region, a clumpy “thin disk”, concentrated in the spiral arms, and a smooth “thick disk” (or flattened “halo”). The emissivity ratio of the two disks seems to be related to the magnetic field properties: Galaxies with strong radio spiral arms reveal a ...
Rainer Beck, Wolfgang Reich
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CO in the Bipolar Radio Continuum Galaxy NGC 3367 [PDF]
The Astronomical Journal, 2005 CO emission has been imaged at 2" resolution in the central 10 kpc of the barred spiral galaxy NGC 3367. This galaxy has bipolar synchrotron lobes out to a radii of 6 kpc, straddling the compact nucleus. The peak molecular emission is in a source of radius 2" (425 pc) centered on the galaxy nucleus.
Garcia-Barreto, J. Antonio +3 more
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