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Hydrogen in the regions of four stellar clusters

Published online by Cambridge University Press:  14 August 2015

H. M. Tovmassian
H. M. Tovmassian*
Affiliation:
Byurakan Astrophysical Observatory, Erevan, Armenia, U.S.S.R.

Extract

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Young clusters of O type and the corresponding stellar associations, together with the associated hydrogen complexes, make up the spiral arms of our Galaxy. Thus the investigation of the distribution of hydrogen and its relation to the clusters is of definite interest.

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. 173 - 176
Copyright
Copyright © Reidel 1970 

References

Menon, T. K.: 1956, Astron. J. 61, 9.CrossRefGoogle Scholar
Raimond, E.: 1966, Bull. Astron. Inst. Netherl. 18, 191.Google Scholar
Tovmasjan, H. M.: 1967, IAU Symposium No. 31, p. 37.Google Scholar