Hostname: page-component-745bb68f8f-lrblm Total loading time: 0 Render date: 2025-01-14T03:51:59.970Z Has data issue: false hasContentIssue false
  • English
  • Français

B. Radio Studies

Published online by Cambridge University Press:  25 April 2016

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.

Several regional surveys of southern HI made with the Argentine 100-m telescope were published (30.155.031). HI and other data were used by Dolidze (30.155. 044) to study the local distribution of gas and star forming regions. The Perseus arm region was the subject of an analogous study by Gerasimenko (34.155.139). Vallée (34.155.005) used rotation measure data from extragalactic sources in the direction of the Perseus arm to determine the magnetic field structure there and to constrain gravitational collapse theories of magnetic compression. HI in the direction of the Puppis window was surveyed by Stacy and Jackson (32.131.277) and used to study the turbulent characteristics of the interstellar medium. HI related to Gould“s Belt was studied by Pöppel and Olano (32.155.024, 33.155.030). Salter (34. 131.014) reviewed radio and other observations pertaining tc Loop I, the North Polar Spur, and considered the influence which this structure might have on the local medium.

Type
Other
Information
Transactions of the International Astronomical Union , Volume 19 , Issue 1 , 1985 , pp. 409 - 416
Copyright
Copyright © Reidel 1985

References

Ardeberg, A., Lindgren, H., Maurice, E.: 1984, IAU Colloquium No. 81 (in press).CrossRefGoogle Scholar
Bhat, C.L., Issa, M.R., Houston, B.P., Mayer, C.J. and Wolfendale, A.W.: 1984,(in preparation).Google Scholar
Elmegreen, B.G.: 1984, IAU Symposium No. 106 (in press).CrossRefGoogle Scholar
Kinman, T.D., Wong-Swanson, Wenz, Harlan: 1984, Astron. J. (in press).Google Scholar
Lynga, G.: 1984, IAU Symposium No. 106 (in press).Google Scholar
Yoshii, Y.: 1984, Astron. J. (submitted).Google Scholar