No CrossRef data available.
Article contents
Mass loss and ΔY/ΔZ ratio
Published online by Cambridge University Press: 12 April 2016
Summary
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.
The ΔY/ΔZ abundance ratio is studied taking into account mass loss from intermediate and massive stars, and the Yz vs. Z relation of Peimbert and Serrano (1980a).
- Type
- Session IX - Effects of Mass Loss on the Interstellar Medium
- Information
- International Astronomical Union Colloquium , Volume 59: Effects of Mass Loss on Stellar Evolution , 1981 , pp. 543 - 549
- Copyright
- Copyright © Reidel 1981
References
Chiosi, C.
1977, in “Chemical and Dynamical evolution of our galaxy”, IAU Coll. 45, ed. Basinska-Greeζik, E. and Mayor, M., p. 61
Google Scholar
Hacyan, S., Dultzin-Hacyan, D., Torres-Peimbert, S., Peim-bert, M.
1976, Rev. Mexicana Astron. Astrof.
1
355
Google Scholar
You have
Access