Results 181 to 190 of about 27,135 (218)
Some of the next articles are maybe not open access.
Related searches:
Related searches:
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.
openaire +2 more sources
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.
openaire +2 more sources
On Stars, Their Evolution and Their Stability
Science, 1984The 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)
openaire +2 more sources
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
openaire +1 more source
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
openaire +1 more source
The evolution of massive stars to explosion
Space Science Reviews, 1994We 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
openaire +1 more source
Properties of massive star evolution
Space Science Reviews, 1994New models of massive stars have been calculated as a part of a project aimed at the construction of an extended grid of stellar tracks for several metallicities, covering all the main evolutionary phases of low, intermediate and massive stars, with updated physics.
openaire +1 more source
Beyond horizontal gene transfer: the role of plasmids in bacterial evolution
Nature Reviews Microbiology, 2021Jerónimo Rodríguez-Beltrán +2 more
exaly
Bacterial defences: mechanisms, evolution and antimicrobial resistance
Nature Reviews Microbiology, 2023William P J Smith +2 more
exaly
Intrahost evolution of the gut microbiota
Nature Reviews Microbiology, 2023Hugo Condessa Barreto, Isabel Gordo
exaly
Diversity and evolution of the animal virome
Nature Reviews Microbiology, 2022Erin Harvey, Edward C Holmes
exaly