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Star formation in the Orion Arm

Published online by Cambridge University Press:  04 August 2017

A. Blaauw*
Affiliation:
Kapteyn Astronomical Institute University of Groningen, The Netherlands

Abstract

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We assemble principal constituents of the morphology of the Orion Arm within 1500 pc as a starting point for the study of progression of star formation.

Type
PART II: COMPOSITION, STRUCTURE AND KINEMATICS
Copyright
Copyright © Reidel 1985 

References

Becker, W., and Fenkart, R.: 1970, in IAU Symposium no. 38, “The Spiral Structure of our Galaxy”, ed. Becker, W. and Contopoulos, G., p. 205 CrossRefGoogle Scholar
Blitz, L.: 1980, in “Giant Molecular Clouds in the Galaxy”, ed. Solomon, P.M. and Edmunds, M.G., p. 1 CrossRefGoogle Scholar
Elmegreen, D.M.: 1980, Ap. J. 242, 528 CrossRefGoogle Scholar
Lucke, P.B., and Hodge, P.W.: 1970, Astron. J. 75, 171 CrossRefGoogle Scholar
Schmidt-Kaler, Th.: 1977, Astron. Astrophys. 54, 771 Google Scholar
Thaddeus, P.: 1982, in “Symposium on the Orion Nebula to honor Henry Draper”, ed. Glassgold, A.E., Huggins, P.J., Schucking, E.L., Ann. New York Acad. Sci. 395, p. 9 CrossRefGoogle Scholar
Tsioumis, A., and Fricke, W.: 1979, Astron. Astrophys. 75, 1 Google Scholar
Wouterloot, J.: 1981, Thesis University of Leiden, ch. VI.Google Scholar