Fine structure in high velocity clouds near the south celestial pole

Details Fine structure in high velocity clouds near the south celestial pole Fine structure in high velocity clouds near the south celestial pole

Nov 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...115..249m&link_type=abstract

Astronomy and Astrophysics, vol. 115, no. 2, Nov. 1982, p. 249-252.

Astronomy and Astrophysics

Astrophysics

19

Hydrogen Clouds, Interstellar Matter, Magellanic Clouds, Molecular Clouds, Relativistic Plasmas, Astronomical Maps, Spatial Distribution, Velocity Measurement

Scientific paper

Three high velocity clouds (HVCs) in the region between the Magellanic Clouds and the Galactic Plane have been mapped in the 21 cm line of neutral hydrogen with the 30 m IAR Radiotelescope. One of these clouds, HVC300(minus)24(plus)274 seems to be connected with the H I gas around the Magellanic Clouds. It could have originated as a part of the same phenomena that created the Magellanic Stream.

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