Authors: Jeffrey Joseph Wolynski
Subdwarf B and O stars are placed on the Wolynski-Taylor Diagram. They are intermediate white dwarfs which are expanding/contracting at regular rates giving the impression that they are pulsing, all the way until they fully expand into O star stages. From then, they will begin cooling and contracting slowly, losing mass and energy becoming the much more highly evolved brown dwarfs, and then to the objects called "planet".
Comments: 2 Pages. 1 diagram
[v1] 2019-01-27 14:17:40
Unique-IP document downloads: 0 times
Vixra.org is a pre-print repository rather than a journal. Articles hosted may not yet have been verified by peer-review and should be treated as preliminary. In particular, anything that appears to include financial or legal advice or proposed medical treatments should be treated with due caution. Vixra.org will not be responsible for any consequences of actions that result from any form of use of any documents on this website.
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.