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Photometric and spectroscopic data for some distant O and B stars
Published online by Cambridge University Press: 14 August 2015
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 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