Growth of isothermal perturbations during and after the recombination era (1986)
- Authors:
- Autor USP: OPHER, REUVEN - IAG
- Unidade: IAG
- Assunto: ASTRONOMIA
- Language: Português
- Source:
- Título do periódico: Revista Mexicana de Astronomia Y Astrofisica
- Volume/Número/Paginação/Ano: v.12, p.38-45, 1986
-
ABNT
ARAUJO, J C N e OPHER, Reuven. Growth of isothermal perturbations during and after the recombination era. Revista Mexicana de Astronomia Y Astrofisica, v. 12, p. 38-45, 1986Tradução . . Acesso em: 28 abr. 2024. -
APA
Araujo, J. C. N., & Opher, R. (1986). Growth of isothermal perturbations during and after the recombination era. Revista Mexicana de Astronomia Y Astrofisica, 12, 38-45. -
NLM
Araujo JCN, Opher R. Growth of isothermal perturbations during and after the recombination era. Revista Mexicana de Astronomia Y Astrofisica. 1986 ;12 38-45.[citado 2024 abr. 28 ] -
Vancouver
Araujo JCN, Opher R. Growth of isothermal perturbations during and after the recombination era. Revista Mexicana de Astronomia Y Astrofisica. 1986 ;12 38-45.[citado 2024 abr. 28 ] - Where does the gravitational energy and angular momentum go in the formation of stars?
- Study of the Casimir energy in an expanding finiteuniverse
- Origem e amplificação de campos magnéticos primordiais
- Studying the decay of the vacuum energy with the observed density power spectrum
- Origin of the intense magnetic fields in magnetars, quasars and GRBS
- Matter density fluctuations in the running 'lâmbda'CDM and 'lâmbda'XCDM models
- Magnetic fields in gamma-ray burst afterglows
- Generalized noncommutative inflation
- Origin of '10 POT. 15 - 10 pot. 16' magnetic fields in the central engine of gamma ray bursts
- Polarized radiation from am herculis binaries
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
