No CrossRef data available.
Article contents
The Formation of Nitrogen and Carbon Lines in HD 50896(WN5)
Published online by Cambridge University Press: 04 August 2017
Extract
Although considerable progress has been made in understanding Wolf-Rayet (WR) stars, the basic mechanisms for producing the nitrogen and carbon emission lines, which characterize a WR's spectrum, are unknown. To determine the mechanisms giving rise to these lines we are currently studying the formation of N and C emission lines in the WN5 star HD 50896.
- Type
- Poster Papers 2
- Information
- Symposium - International Astronomical Union , Volume 116: Luminous Stars and Associations in Galaxies , 1986 , pp. 261 - 264
- Copyright
- Copyright © Reidel 1986