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físico indio Subrahmanyan Chandrasekhar (1910–1995), descubrió y publicó en 1942 el denominado límite Schönberg-Chandrasekhar, que es la máxima masa del…8 kB (827 palabras) - 03:00 8 mar 2024
circundante, hay una masa máxima llamada límite de Schönberg–Chandrasekhar. Cuando la masa supera este límite, el núcleo se colapsa y las capas externas…16 kB (2044 palabras) - 19:02 23 ago 2023
Resultados de la Wikipedia en inglés.
- In stellar astrophysics, the Schönberg–Chandrasekhar limit is the maximum mass of a non-fusing, isothermal core that can support an enclosing envelope…3 kB (446 palabras) - 03:57 24 ene 2020
- The Chandrasekhar limit (/ˌtʃændrəˈʃeɪkər/) is the maximum mass of a stable white dwarf star. The currently accepted value of the Chandrasekhar limit is…34 kB (3933 palabras) - 02:21 3 may 2024
- Mário Schenberg (redirección desde Mario Schönberg)physicist Subrahmanyan Chandrasekhar (1910–1995), he discovered and published in 1942 the so-called Schönberg–Chandrasekhar limit, which is the maximum…9 kB (902 palabras) - 01:20 11 abr 2024
- and inventions, including the Chandrasekhar limit and the Chandra X-Ray Observatory, are named after him. Chandrasekhar worked on a wide variety of problems…60 kB (5701 palabras) - 04:59 3 may 2024
- H-function Schönberg–Chandrasekhar limit Velikhov–Chandrasekhar instability Batchelor–Chandrasekhar equation Chandrasekhar–Page equations Chandrasekhar's white…1 kB (79 palabras) - 18:45 21 mar 2022
- is still below the Schönberg–Chandrasekhar limit, but hydrogen shell fusion quickly increases the mass of the core beyond that limit. More-massive stars…29 kB (3699 palabras) - 23:28 24 mar 2024
- S2CID 119239346. Ball, Warrick H. (2012). "Quasi-stars and the Schönberg-Chandrasekhar limit". arXiv:1207.5972. Czerny, Bozena; Janiuk, Agnieszka; Sikora…9 kB (1048 palabras) - 10:20 18 abr 2024
- shell, there is a maximum mass called the Schönberg–Chandrasekhar limit. When the mass exceeds that limit, the core collapses, and the outer layers of…15 kB (1845 palabras) - 05:26 29 ene 2024
- Instead, after just a few million years the core reaches the Schönberg–Chandrasekhar limit, rapidly collapses, and may become degenerate. This causes the…16 kB (2321 palabras) - 14:49 20 abr 2024
- largely of helium. The mass of the helium core is below the Schönberg–Chandrasekhar limit and is in thermal equilibrium, and the star is a subgiant. Any…32 kB (3933 palabras) - 15:04 20 nov 2023
- longer in thermal equilibrium, either degenerate or above the Schönberg–Chandrasekhar limit, so it increases in temperature which causes the rate of fusion…49 kB (6424 palabras) - 20:50 5 mar 2024
- N. Zytkow, Nidia Morrell: [4] Quasi-stars, giants and the Schönberg–Chandrasekhar (SC) limit; Monthly Notices of the Royal Astronomical Society; January…13 kB (1228 palabras) - 00:09 30 nov 2023