Hostname: page-component-cd9895bd7-8ctnn Total loading time: 0 Render date: 2024-12-25T17:21:53.444Z Has data issue: false hasContentIssue false
  • English
  • Français

Star Chains and Dark Filaments in Galactic Nebulae

Published online by Cambridge University Press:  03 August 2017

V. G. Fessenkov
V. G. Fessenkov*
Affiliation:
Astrophysical Institute, Alma-Ata, U.S.S.R.

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

When investigating sufficiently dense star fields, one often finds some short chains of stars oriented with a certain regularity and in a few cases connected with dark filaments of the galactic nebulae. It is necessary to be very cautious in the interpretation of this phenomenon, because even completely accidental clustering of some objects can sometimes lead to interesting deviations from homogeneity.

Type
Part I: Empirical Studies of Velocity Fields in, and Related Structure of, the Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 8: Cosmical Gas Dynamics , July 1958 , pp. 951 - 952
Copyright
Copyright © American Physical Society 1958 

References

1 Martynov, D. J., Astron. Circ. N 149 (1954).Google Scholar