Hostname: page-component-7bb8b95d7b-lvwk9 Total loading time: 0 Render date: 2024-09-05T23:59:41.409Z Has data issue: false hasContentIssue false
  • English
  • Français

A Search for Low-Velocity Neutral Hydrogen in the Magellanic Stream

Published online by Cambridge University Press:  04 August 2017

N. V. Bystrova
N. V. Bystrova*
Affiliation:
Leningrad Branch of the Special, Astrophysical Observatory, USSR Academy of Sciences

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The large velocity range of the HI clouds belonging to the Magellanic Stream, as found by Haynes (1979), makes it reasonable to search for some low LSR velocity neutral hydrogen possibly belonging to the Stream. This gas, if any, would be severely blended by the local galactic gas.

Type
Dynamics
Information
Symposium - International Astronomical Union , Volume 108: Structure and Evolution of the Magellanic Clouds , 1984 , pp. 139 - 140
Copyright
Copyright © Reidel 1984 

References

Bystrova, N.V., Rakhimov, I.A.: 1977, Pulkovo Sky Survey in the interstellar neutral Hydrogen Radio Line, “Nauka”, Leningrad Google Scholar
Bystrova, N.V.: 1980, Contour maps to the Pulkovo Sky Survey in the interstellar neutral Hydrogen Radio Line, “Nauka”, Leningrad Google Scholar
Cohen, R.J.: 1982, Mon. Not. R. astr. Soc. 199, 281 Google Scholar
Haynes, M.P.: 1979, Astron. J. 84, 1173 Google Scholar
Wannier, P., Wrixon, G.T.: 1972, Ap. J. 173, L 119 Google Scholar