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Contribution to the study of the distribution of neutral hydrogen in the region 230° ≤ lII ≤ 280°
Published online by Cambridge University Press: 14 August 2015
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° ≤ lII ≤ 280°, −15° ≤ bII ≤ −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 lII = 265°. We also study the concentrations which lie far below the plane; some of them seem to be related to Lindblad's G arm.
- Type
- Part II/Observations of Spiral Structure in Our Galaxy
- Information
- Symposium - International Astronomical Union , Volume 38: The Spiral Structure of our Galaxy , 1970 , pp. 157 - 163
- Copyright
- Copyright © Reidel 1970