Population III Supernovae and the formation of galaxies (1997)
- Autores:
- Autor USP: OPHER, REUVEN - IAG
- Unidade: IAG
- Assuntos: ASTRONOMIA; GALÁXIAS; ASTROFÍSICA
- Idioma: Inglês
- Imprenta:
- Editora: Astronomical Society of the Pacific
- Local: San Francisco
- Data de publicação: 1997
- Fonte:
- Título do periódico: Proceedings
- Nome do evento: Workshop Young Galaxies and Qso Absorption-Line Systems
-
ABNT
MIRANDA, Oswaldo D e OPHER, Reuven. Population III Supernovae and the formation of galaxies. 1997, Anais.. San Francisco: Astronomical Society of the Pacific, 1997. . Acesso em: 19 set. 2024. -
APA
Miranda, O. D., & Opher, R. (1997). Population III Supernovae and the formation of galaxies. In Proceedings. San Francisco: Astronomical Society of the Pacific. -
NLM
Miranda OD, Opher R. Population III Supernovae and the formation of galaxies. Proceedings. 1997 ;[citado 2024 set. 19 ] -
Vancouver
Miranda OD, Opher R. Population III Supernovae and the formation of galaxies. Proceedings. 1997 ;[citado 2024 set. 19 ] - Producing superhearvy dark matter during inflation
- The missing mass problem in galaxy clusters and mond
- Magnetic fields and the first objects
- Limitation of the decay of the vacuum energy by observations
- Introduction to the Seventh Brazilian Workshop on New Physics from Space
- Origin of '10 POT. 15 - 10 POT. 16' G magnetic fields in the central engine of gamma ray bursts
- The origin of magnetic fields in galaxies
- Decrease in the number of small dark matter haloes due to oscillations in the inflaton potential
- Decrease in the number of small dark matter haloes due to oscillations in the inflation potential
- Introduction to the Tenth Brazilian Workshop on New Physics from Space
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