Relativistic evolution of 103 M &sun; star

Details Relativistic evolution of 103 M &sun; star Relativistic evolution of 103 M &sun; star

Dec 1971

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1971ap%26ss..14..378k&link_type=abstract

Astrophysics and Space Science, Volume 14, Issue 2, pp.378-388

Astronomy and Astrophysics

Astrophysics

6

Scientific paper

A fully relativistic evolution of 103 M &sun; is described for initial composition ofY=Z=0. Our results show that (a) a great part of the star is in radiative equilibrium, (b) the maximal red-shift for main-sequence 103 M &sun; stars is significantly less than for isentropic models, and (c) a very low amount of CNO elements (<10-8 by mass) is formed at any stage before hydrogen is completely consumed and hence such stars cannot be the progenitors of Population II stars.

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