H I Emission and Absorption in the Southern Galactic Plane
Survey¹
N. M. McClure-Griffiths ,
John M. Dickey ,
B. M. Gaensler ,
A. J. Green ,
R. F. Haynes ,
M. H. Wieringa
, PASA, 18 (1), in press.

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Conclusions

New large-scale, high-resolution H I surveys like the SGPS and CGPS finally make it possible to simultaneously study the small and large scale structure of the ISM. We hope that the SGPS dataset will allow us to understand how the large and small scale structures relate to each other throughout the inner Galaxy. The SGPS should be able to catalogue the majority of HI shells in the inner Galaxy and determine exactly how they shape the ISM. It is likely that we are currently seeing only the most dramatic cold clouds with HISA, however further studies may lead to a complete understanding the distribution of the CNM.

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Next Section: Acknowledgements
Title/Abstract Page: H I Emission and Absorption
Previous Section: Questions and Future Work
Contents Page: Volume 18, Number 1

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© Copyright Astronomical Society of Australia 1997