The Beginning of Homogeneous Nucleation of Iron/Nickel Cores in Homogeneous Young Stars

Authors: Jeffrey Joseph Wolynski

To begin the process of forming homogeneous iron/nickel cores it is required that the young, hot stars be homogeneous in their interiors. To form an iron/nickel core as the star evolves, no nuclear core can be present. It would be too hot for the iron/nickel vapor to clump together and it would get in the way of the differentiation process.

Comments: 1 Page.

Download: PDF

Submission history

[v1] 2017-04-13 22:15:25

Unique-IP document downloads: 6 times

Add your own feedback and questions here:
You are equally welcome to be positive or negative about any paper but please be polite. If you are being critical you must mention at least one specific error, otherwise your comment will be deleted as unhelpful.

comments powered by Disqus