Abstract
A sky survey of the 21 cm hydrogen line has been made with the 100-foot Radiotelescope of the I.A.R.-C.I.W. Radio Astronomy Station in the region 230° ≤ l II ≤ 280°, −15° ≤ b II ≤ −3°.
We study the distribution of the local hydrogen and that in the Orion, Intermediate and Perseus arms. We find a new structure that starts at l II = 265°. We also study the concentrations which lie far below the plane; some of them seem to be related to Lindblad’s G arm.
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© 1970 I.A.U.
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Goniadzki, D., Jech, A. (1970). Contribution to the Study of the Distribution of Neutral Hydrogen in the Region 230°≤l II≤280°. In: Becker, W., Contopoulos, G. (eds) The Spiral Structure of Our Galaxy. International Astronomical Union / Union Astronomique Internationale, vol 38. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-3275-9_26
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DOI: https://doi.org/10.1007/978-94-010-3275-9_26
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-3277-3
Online ISBN: 978-94-010-3275-9
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