Influence of the Black Hole Rotation on Accretion Discs and Jets in Active Galaxies: the Case of NGC 1068
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| Format: | Artículo científico |
| Langue: | en |
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Sociedade Brasileira de Física
2005
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| _version_ | 1876472548395319296 |
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| author | Anderson Caproni |
| author_facet | Anderson Caproni |
| contents | Influence of the Black Hole Rotation on Accretion Discs and Jets in Active Galaxies: the Case of NGC 1068 Anderson Caproni Herman J. Mosquera Cuesta Zulema Abraham Física, Astronomía y Matemáticas Although we do not observe directly black holes in the Universe, their presence has been inferred in severalastrophysical systems, from galactic to extragalactic scales. In this work, we will restrict our focus in thepossible signatures of the presence of Kerr black holes in active galactic nuclei, one of the most powerfulsources in the Universe. Particularly, we will discuss how jet/accretion disc precession and their directionalstability can be used to trace the accretion disc properties as well as the black hole spin in the Seyfert galaxyNGC1068. 2005 artículo científico 0103-9733 https://www.redalyc.org/articulo.oa?id=46435744 en http://www.redalyc.org/revista.oa?id=464 Brazilian Journal of Physics application/pdf Sociedade Brasileira de Física Brazilian Journal of Physics (Brasil) Num.4B Vol.35 |
| format | Artículo científico |
| id | redalyc_46435744 |
| institution | Redalyc |
| language | en |
| publishDate | 2005 |
| publisher | Sociedade Brasileira de Física |
| spellingShingle | Influence of the Black Hole Rotation on Accretion Discs and Jets in Active Galaxies: the Case of NGC 1068 Anderson Caproni Física, Astronomía y Matemáticas Influence of the Black Hole Rotation on Accretion Discs and Jets in Active Galaxies: the Case of NGC 1068 Anderson Caproni Herman J. Mosquera Cuesta Zulema Abraham Física, Astronomía y Matemáticas Although we do not observe directly black holes in the Universe, their presence has been inferred in severalastrophysical systems, from galactic to extragalactic scales. In this work, we will restrict our focus in thepossible signatures of the presence of Kerr black holes in active galactic nuclei, one of the most powerfulsources in the Universe. Particularly, we will discuss how jet/accretion disc precession and their directionalstability can be used to trace the accretion disc properties as well as the black hole spin in the Seyfert galaxyNGC1068. 2005 artículo científico 0103-9733 https://www.redalyc.org/articulo.oa?id=46435744 en http://www.redalyc.org/revista.oa?id=464 Brazilian Journal of Physics application/pdf Sociedade Brasileira de Física Brazilian Journal of Physics (Brasil) Num.4B Vol.35 |
| title | Influence of the Black Hole Rotation on Accretion Discs and Jets in Active Galaxies: the Case of NGC 1068 |
| topic | Física, Astronomía y Matemáticas |
| url | https://www.redalyc.org/articulo.oa?id=46435744 |