Stationary Relativistic Magnetic Jets from Black Holes
Abstract We investigate the jet formation region of relativistic magnetic jetsusing stationary axisymmetric MHD models.We numerically calculate the field structure of the collimating jetand the flow acceleration. Special or general relativistic effects areconsidered. Stationarity allows for a global...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Fendt, Christian [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
2001 |
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| Schlagwörter: |
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| Anmerkung: |
© Kluwer Academic Publishers 2001 |
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| Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 276(2001), Suppl 1 vom: Jan., Seite 297-299 |
|---|---|
| Übergeordnetes Werk: |
volume:276 ; year:2001 ; number:Suppl 1 ; month:01 ; pages:297-299 |
| Links: |
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| DOI / URN: |
10.1023/A:1011634200147 |
|---|
| Katalog-ID: |
OLC2066225592 |
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| 520 | |a Abstract We investigate the jet formation region of relativistic magnetic jetsusing stationary axisymmetric MHD models.We numerically calculate the field structure of the collimating jetand the flow acceleration. Special or general relativistic effects areconsidered. Stationarity allows for a global treatment of the jetphysics. Our results are applicable to highly relativistic jets of AGNand microquasars. | ||
| 650 | 4 | |a Black Hole | |
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| 650 | 4 | |a Flow Acceleration | |
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10.1023/A:1011634200147 doi (DE-627)OLC2066225592 (DE-He213)A:1011634200147-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Fendt, Christian verfasserin aut Stationary Relativistic Magnetic Jets from Black Holes 2001 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2001 Abstract We investigate the jet formation region of relativistic magnetic jetsusing stationary axisymmetric MHD models.We numerically calculate the field structure of the collimating jetand the flow acceleration. Special or general relativistic effects areconsidered. Stationarity allows for a global treatment of the jetphysics. Our results are applicable to highly relativistic jets of AGNand microquasars. Black Hole Relativistic Effect Formation Region Field Structure Flow Acceleration Memola, Elisabetta aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 276(2001), Suppl 1 vom: Jan., Seite 297-299 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:276 year:2001 number:Suppl 1 month:01 pages:297-299 https://doi.org/10.1023/A:1011634200147 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 AR 276 2001 Suppl 1 01 297-299 |
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10.1023/A:1011634200147 doi (DE-627)OLC2066225592 (DE-He213)A:1011634200147-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Fendt, Christian verfasserin aut Stationary Relativistic Magnetic Jets from Black Holes 2001 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2001 Abstract We investigate the jet formation region of relativistic magnetic jetsusing stationary axisymmetric MHD models.We numerically calculate the field structure of the collimating jetand the flow acceleration. Special or general relativistic effects areconsidered. Stationarity allows for a global treatment of the jetphysics. Our results are applicable to highly relativistic jets of AGNand microquasars. Black Hole Relativistic Effect Formation Region Field Structure Flow Acceleration Memola, Elisabetta aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 276(2001), Suppl 1 vom: Jan., Seite 297-299 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:276 year:2001 number:Suppl 1 month:01 pages:297-299 https://doi.org/10.1023/A:1011634200147 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 AR 276 2001 Suppl 1 01 297-299 |
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10.1023/A:1011634200147 doi (DE-627)OLC2066225592 (DE-He213)A:1011634200147-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Fendt, Christian verfasserin aut Stationary Relativistic Magnetic Jets from Black Holes 2001 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2001 Abstract We investigate the jet formation region of relativistic magnetic jetsusing stationary axisymmetric MHD models.We numerically calculate the field structure of the collimating jetand the flow acceleration. Special or general relativistic effects areconsidered. Stationarity allows for a global treatment of the jetphysics. Our results are applicable to highly relativistic jets of AGNand microquasars. Black Hole Relativistic Effect Formation Region Field Structure Flow Acceleration Memola, Elisabetta aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 276(2001), Suppl 1 vom: Jan., Seite 297-299 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:276 year:2001 number:Suppl 1 month:01 pages:297-299 https://doi.org/10.1023/A:1011634200147 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 AR 276 2001 Suppl 1 01 297-299 |
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10.1023/A:1011634200147 doi (DE-627)OLC2066225592 (DE-He213)A:1011634200147-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Fendt, Christian verfasserin aut Stationary Relativistic Magnetic Jets from Black Holes 2001 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2001 Abstract We investigate the jet formation region of relativistic magnetic jetsusing stationary axisymmetric MHD models.We numerically calculate the field structure of the collimating jetand the flow acceleration. Special or general relativistic effects areconsidered. Stationarity allows for a global treatment of the jetphysics. Our results are applicable to highly relativistic jets of AGNand microquasars. Black Hole Relativistic Effect Formation Region Field Structure Flow Acceleration Memola, Elisabetta aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 276(2001), Suppl 1 vom: Jan., Seite 297-299 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:276 year:2001 number:Suppl 1 month:01 pages:297-299 https://doi.org/10.1023/A:1011634200147 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 AR 276 2001 Suppl 1 01 297-299 |
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10.1023/A:1011634200147 doi (DE-627)OLC2066225592 (DE-He213)A:1011634200147-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Fendt, Christian verfasserin aut Stationary Relativistic Magnetic Jets from Black Holes 2001 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2001 Abstract We investigate the jet formation region of relativistic magnetic jetsusing stationary axisymmetric MHD models.We numerically calculate the field structure of the collimating jetand the flow acceleration. Special or general relativistic effects areconsidered. Stationarity allows for a global treatment of the jetphysics. Our results are applicable to highly relativistic jets of AGNand microquasars. Black Hole Relativistic Effect Formation Region Field Structure Flow Acceleration Memola, Elisabetta aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 276(2001), Suppl 1 vom: Jan., Seite 297-299 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:276 year:2001 number:Suppl 1 month:01 pages:297-299 https://doi.org/10.1023/A:1011634200147 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 AR 276 2001 Suppl 1 01 297-299 |
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Abstract We investigate the jet formation region of relativistic magnetic jetsusing stationary axisymmetric MHD models.We numerically calculate the field structure of the collimating jetand the flow acceleration. Special or general relativistic effects areconsidered. Stationarity allows for a global treatment of the jetphysics. Our results are applicable to highly relativistic jets of AGNand microquasars. © Kluwer Academic Publishers 2001 |
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Abstract We investigate the jet formation region of relativistic magnetic jetsusing stationary axisymmetric MHD models.We numerically calculate the field structure of the collimating jetand the flow acceleration. Special or general relativistic effects areconsidered. Stationarity allows for a global treatment of the jetphysics. Our results are applicable to highly relativistic jets of AGNand microquasars. © Kluwer Academic Publishers 2001 |
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Abstract We investigate the jet formation region of relativistic magnetic jetsusing stationary axisymmetric MHD models.We numerically calculate the field structure of the collimating jetand the flow acceleration. Special or general relativistic effects areconsidered. Stationarity allows for a global treatment of the jetphysics. Our results are applicable to highly relativistic jets of AGNand microquasars. © Kluwer Academic Publishers 2001 |
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