Abstract
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 l II = 298°.
This is a preview of subscription content, log in via an institution to check access.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
Alter, G., Hogg, H. S., Ruprecht, J., and Vanÿsek, V.: 1959, Bull. Astron. Inst. Csz. 10, Appendix, p. 1.
Blaauw, A.: 1963, Stars and Stellar Systems 3, 383.
Feast, M. W.: 1967, Monthly Notices Roy. Astron. Soc. 136, 141.
Gollnow, H.: 1962, Monthly Notices Roy. Astron. Soc. 123, 391.
Johnson, H. L.: 1963, Stars and Stellar Systems, 3, 204.
Kraft, R. P. and Schmidt, M.: 1963, Astrophys. J. 137, 249.
Lindholm, E. H.: 1957, Astrophys. J. 126, 588.
Lyngâ, G.: 1968, Medd. Lunds Astron. Obs., Ser. I, No. 238.
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1970 I.A.U.
About this chapter
Cite this chapter
Lyngå, G. (1970). Photometric and Spectroscopic Data for Some Distant O and B Stars. In: Becker, W., Contopoulos, G. (eds) The Spiral Structure of Our Galaxy. International Astronomical Union / Union Astronomique Internationale, vol 38. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-3275-9_47
Download citation
DOI: https://doi.org/10.1007/978-94-010-3275-9_47
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-3277-3
Online ISBN: 978-94-010-3275-9
eBook Packages: Springer Book Archive