No CrossRef data available.
Article contents
Radial Velocity of the Central Star of NGC 1514
Published online by Cambridge University Press: 14 August 2015
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.
We would like to report on some spectroscopic observations made of the central star of the planetary nebula NGC 1514, which we think can support the binary hypothesis now advanced by Kohoutek.
- Type
- Session V – Central Stars
- Information
- Copyright
- Copyright © Reidel 1968
You have
Access