Hostname: page-component-586b7cd67f-t8hqh Total loading time: 0 Render date: 2024-11-29T11:07:13.835Z Has data issue: false hasContentIssue false
  • English
  • Français

Photometric and spectroscopic data for some distant O and B stars

Published online by Cambridge University Press:  14 August 2015

G. Lyngå
G. Lyngå*
Affiliation:
Lund Observatory, Lund, Sweden

Abstract

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.

The open cluster Stock 16 and some distant OB stars in Crux have been studied. Lack of absorption between spiral arms -I and -II is apparent. Negative residual radial velocities are found at distances of about 6 kpc at lII = 298°.

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. 270 - 275
Copyright
Copyright © Reidel 1970 

References

Alter, G., Hogg, H. S., Ruprecht, J., and Vanýsek, V.: 1959, Bull. Astron. Inst. Csz. 10, Appendix, p. 1.Google Scholar
Blaauw, A.: 1963, Stars and Stellar Systems 3, 383.Google Scholar
Feast, M. W.: 1967, Monthly Notices Roy. Astron. Soc. 136, 141.Google Scholar
Gollnow, H.: 1962, Monthly Notices Roy. Astron. Soc. 123, 391.Google Scholar
Johnson, H. L.: 1963, Stars and Stellar Systems 3, 204.Google Scholar
Kraft, R. P. and Schmidt, M.: 1963, Astrophys. J. 137, 249.CrossRefGoogle Scholar
Lindholm, E. H.: 1957, Astrophys. J. 126, 588.Google Scholar
Lyngå, G.: 1968, Medd. Lunds Astron. Obs., Ser. I, No. 238.Google Scholar