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New high-sensitivity observations of the Magellanic Stream have been carried out from the Instituto Argentino de Radioastronomia. The Stream was surveyed between dec. -44 deg and -20 deg. The data are presented in the form of maps of H I column density distribution and velocity distribution.
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Magellanic Stream: A Possible Tool for Studying Dark Halo Model [PDF]
We model the dynamics of Magellanic Stream with the ram-pressure scenario in the logarithmic and power-law galactic halo models and construct numerically the past orbital history of Magellanic clouds and Magellanic Stream. The parameters of models include the asymptotic rotation velocity of spiral arms, halo flattening, core radius and rising or ...
arxiv
Observations of a Magellanic Corona. [PDF]
Krishnarao D+8 more
europepmc +1 more source
CLSoilMaps: A national soil gridded database of physical and hydraulic soil properties for Chile. [PDF]
Dinamarca DI+3 more
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Anaesthetic management and complications of a Humboldt penguin (Spheniscus humboldti) undergoing diagnostic imaging. [PDF]
Romero P+4 more
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A Possible New Segment of the Magellanic Stream in the Northern Sky [PDF]
R. J. Cohen, R. D. Davies
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The Magellanic stream - The turbulent wake of the Magellanic clouds in the halo of the Galaxy
New observations of the Magellanic Stream were made in December 1976 with the 64-m radio telescope at the Parkes Observatory of CSIRO. The ridges of H I emission of the Stream were traced from near its tip at ℓ = 90°, b = -40° to the Magellanic Clouds.
J. D. Murray+2 more
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Velocity structure in the Magellanic Stream
New high sensitivity neutral hydrogen observations of the area of the south galactic pole reveal that the region is littered with anomalous velocity clouds, both positive and negative. It is suggested that all of these clouds are associated with the Magellanic Stream phenomenon.
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The Magellanic Stream and the Density of Coronal Gas in the Galactic Halo [PDF]
Chigurupati Murali
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A helium-burning white dwarf binary as a supersoft X-ray source. [PDF]
Greiner J+14 more
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