Can the filaments of the radio sources be really due to synchrotron thermal instabilities? (1993)
- Authors:
- USP affiliated authors: PINO, ELISABETE MARIA DE GOUVEIA DAL - IAG ; OPHER, REUVEN - IAG
- Unidade: IAG
- Subjects: ASTRONOMIA; ASTROFÍSICA
- Language: Inglês
- Imprenta:
- Publisher: Cambridge University
- Publisher place: Cambridge
- Date published: 1993
- Conference titles: Nuffield Radio Astronomy Laboratories' Conference
-
ABNT
GOUVEIA DAL PINO, Elisabete Maria de e OPHER, Reuven. Can the filaments of the radio sources be really due to synchrotron thermal instabilities? 1993, Anais.. Cambridge: Cambridge University, 1993. . Acesso em: 03 mar. 2026. -
APA
Gouveia dal Pino, E. M. de, & Opher, R. (1993). Can the filaments of the radio sources be really due to synchrotron thermal instabilities? In . Cambridge: Cambridge University. -
NLM
Gouveia dal Pino EM de, Opher R. Can the filaments of the radio sources be really due to synchrotron thermal instabilities? 1993 ;[citado 2026 mar. 03 ] -
Vancouver
Gouveia dal Pino EM de, Opher R. Can the filaments of the radio sources be really due to synchrotron thermal instabilities? 1993 ;[citado 2026 mar. 03 ] - Formation of filaments in the crab nebula by a thermal synchrotron instabilyty
- 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
- Are the filaments formed by synchrotron thermal instability bright?
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