No CrossRef data available.
Article contents
Outer Disc Rotation from Cepheid Variables
Published online by Cambridge University Press: 25 May 2016
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.
We have measured radial velocities for a large number of classical cepheids of the Galaxy, particularly in the outer disc. We determine the rotation curve up to a galactocentric radius of 16 kpc. The results are then compared to similar studies using HII regions. We also consider some possible complications.
- Type
- Chapter 8: How do we put it together?
- Information
- Symposium - International Astronomical Union , Volume 169: Unsolved Problems of the Milky Way , 1996 , pp. 661 - 667
- Copyright
- Copyright © Kluwer 1996