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The evolution of the stars

Mathematical Proceedings of the Cambridge Philosophical Society, 1939
Difficulties associated with the evolution of stars by radiation alone are briefly discussed. It is clear that some other process is also affecting the stars and it is shown that the stars are capable of adding to their mass by the process of accretion of the cosmical cloud.
Hoyle, F., Lyttleton, R. A.
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On Stars, Their Evolution and Their Stability

Science, 1984
The Nobel lecture of Chandrasekhar is printed in which he describes the basic processes that determine the life history of a star with particular emphasis on the roles of stellar mass and radiation pressure. (AIP)
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Evolution of massive stars

1989
The term massive star is not very precise, and in the following we shall use it for stars with zero age main sequence (ZAMS) masses M ZAMS above approximately 15 M ⊙. Note, however, that these abjects may achieve actual masses well below 15 M ⊙ during their evolution, as a consequence of mass loss due to stellar winds, pulsations, or other processes. M
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The evolution of massive stars to explosion

Space Science Reviews, 1994
We review the possible evolutionary paths from massive stars to explosive endpoints as various types of supernovae associated with Population I and hence with massive stars: Type II-P, Type II-L, Type Ib, Type Ic, and the hybrid events SN 1987K and SN 1993J.
J. C. Wheeler, D. A. Swartz
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Beyond horizontal gene transfer: the role of plasmids in bacterial evolution

Nature Reviews Microbiology, 2021
Jeronimo Rodríguez-Beltrán   +2 more
exaly  

Bacterial defences: mechanisms, evolution and antimicrobial resistance

Nature Reviews Microbiology, 2023
William P J Smith   +2 more
exaly  

Intrahost evolution of the gut microbiota

Nature Reviews Microbiology, 2023
Hugo C Barreto   +2 more
exaly  

Diversity and evolution of the animal virome

Nature Reviews Microbiology, 2022
Erin Harvey   +2 more
exaly  

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