The Evolution of Massive Stars Initially Composed of Pure Hydrogen
R Van Der Borght
Australian Journal of Physics
17(2) 165 - 174
Published: 1964
Abstract
The object of the present paper is to investigate the influence of carbon abundance on the evolution of the massive stars, initially composed of pure hydrogen, during the pre-main-sequence contraction and the hydrogen burning phase of these stars_https://doi.org/10.1071/PH640165
© CSIRO 1964
