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Space distribution of interstellar dust in connection with the galactic spiral structure

Published online by Cambridge University Press:  14 August 2015

T. A. Uranova
T. A. Uranova*
Affiliation:
Moscow University, Moscow, U.S.S.R.

Abstract

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A maximum of dust density along the inner edge of the Cygnus arm is found. It seems that the same happens along the inner edges of the Perseus and the Sagittarius arms.

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. 228 - 231
Copyright
Copyright © Reidel 1970 

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