Formation of condensation in extended and compact radio sources and stellar winds (1988)
- Authors:
- USP affiliated authors: PINO, ELISABETE MARIA DE GOUVEIA DAL - IAG ; OPHER, REUVEN - IAG
- Unidade: IAG
- Assunto: ASTRONOMIA
- Language: Português
- Imprenta:
- Publisher: American Physical Society
- Publisher place: Santa Fe
- Date published: 1988
- Source:
- Título: Proceedings
- Conference titles: Topical Conference on Plasma Astrophysics
-
ABNT
GOUVEIA DAL PINO, Elisabete Maria de e OPHER, Reuven. Formation of condensation in extended and compact radio sources and stellar winds. 1988, Anais.. Santa Fe: American Physical Society, 1988. . Acesso em: 15 mar. 2026. -
APA
Gouveia dal Pino, E. M. de, & Opher, R. (1988). Formation of condensation in extended and compact radio sources and stellar winds. In Proceedings. Santa Fe: American Physical Society. -
NLM
Gouveia dal Pino EM de, Opher R. Formation of condensation in extended and compact radio sources and stellar winds. Proceedings. 1988 ;[citado 2026 mar. 15 ] -
Vancouver
Gouveia dal Pino EM de, Opher R. Formation of condensation in extended and compact radio sources and stellar winds. Proceedings. 1988 ;[citado 2026 mar. 15 ] - Formation of filaments in the crab nebula by a thermal synchrotron instabilyty
- Can the filaments of the radio sources be really due to synchrotron thermal instabilities?
- Are the observed filaments in extend radio sources due to synchrotron radiation thermal instabilities
- Origem dos nos em radiafontes compactas superluminais
- Possible origin of the superluminal knots
- Energy spectrum of the filaments formed by synchrotron thermal instability in radio sources
- Origin of the filaments in the crab nebula
- Formation of condensations in young stellar outflows by a thermal instability
- Distribuição da energia eletrônica e da luminosidade espectral nas condensações formadas por instabilidade térmica sincrotron-compton-inverso em radiofontes
- Spectral luminosity and the electron energy distribution in condensations formed by the synchrotron inverse - compton thermal instability
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