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Infall of HVC's and the Origin of HI Supershells

Published online by Cambridge University Press:  03 August 2017

I.F. Mirabel
I.F. Mirabel*
Affiliation:
Service D'Astrophysique, CEA-CEN. Saclay, 91191 Gif sur Yvette, FRANCE

Abstract

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Surveys for atomic hydrogen at very high velocities (|V| ≥ 140 km s–1) in the galactic center and anticenter regions of the sky reveal a net inflow of gas toward the Milky Way. In the anticenter, the collisions of infalling clouds with galactic material trigger the most energetic structural disturbance in the Galaxy, the “anticenter supershell”.

Type
I. The Disk-Halo Interface in Our Galaxy
Information
Symposium - International Astronomical Union , Volume 144: The Interstellar Disk-Halo Connection in Galaxies , 1991 , pp. 89 - 91
Copyright
Copyright © Kluwer 1991 

References

REFERENCES

Heiles, C. (1979) Astrophys. J. 55, 585 CrossRefGoogle Scholar
Hulsbosch, A.N.M., Wakker, B.R (1988) Astron. Ap. Supp 75, 191 Google Scholar
Kulkarni, S.R., Mathieu, R. (1986) Ap. Space Sci. 118, 531 CrossRefGoogle Scholar
Mirabel, I.F. (1989) in Structure and Dynamics of the Interstellar Medium , eds. Tenorio-Tagle, G., Moles, M., Melnick, J., p. 396 Google Scholar
Mirabel, I.F., Morras, R. (1984) Astrophys. J. , 279, 86 CrossRefGoogle Scholar
Mirabel, I.F., Morras, R. (1990) Astrophys. J. 356, 130 CrossRefGoogle Scholar
Oort, J.H. (1970) Astr. Ap. 7, 381 Google Scholar
Tenorio- Tagle, G. (1980) Astron. Ap. 88, 61 Google Scholar