Zobrazeno 1 - 10
of 24
pro vyhledávání: '"circumnuclear matter"'
Autor:
Bučar Bricman, Katja
Tidal Disruption Events (TDEs) are rare transients, which are considered to be promising tools in probing supermassive black holes (SMBHs) and their environments in quiescent galaxies, accretion physics, and jet formation mechanisms. The majority of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3507::c35459d11c45db044db32f3d4ee1f08b
http://repozitorij.ung.si/Dokument.php?id=23875&dn=
http://repozitorij.ung.si/Dokument.php?id=23875&dn=
Autor:
Clerici, Aurora
The number of observed tidal disruption events is increasing rapidly with the advent of new surveys. Thus, it is becoming increasingly important to improve TDE models using different stellar and orbital parameters. We study the dynamical behaviour of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3507::25668f140e4ec33e9240822732515850
https://hdl.handle.net/20.500.12556/RUNG-5853
https://hdl.handle.net/20.500.12556/RUNG-5853
Autor:
Marshall, Herman
I will present a summary of results from 16 years of high resolution X-ray spectroscopy of gas in the neighborhood of Active Galactic Nuclei. Led by the prototypical Sy 2 galaxy NGC 1068, we now have many examples of circumnuclear gas that is excited
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e930f973b477c0fe2083835cc61ece86
Autor:
Daniele Fargion
Earliest AUGER UHECR anisotropy correlated with AGN within a GZK Universe almost fade away. Recent UHECR mass compositions did show a negligible nucleon composition and an UHECR nuclei (light or heavy) signature. The absence of UHECR events toward th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::703c5c776357eac1c248ea896b0156cb
http://arxiv.org/abs/1112.6388
http://arxiv.org/abs/1112.6388
Autor:
Mazzalay, Ximena
Publikováno v:
Repositorio Digital Universitario (UNC)
Universidad Nacional de Córdoba
instacron:UNC
Universidad Nacional de Córdoba
instacron:UNC
Tesis (Doctor en Astronomía)--Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física, 2010. Los núcleos activos de galaxias o AGNs son considerados los objetos más luminosos del Universo. Estos emiten cantidades important
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3056::265375d8320c31cca3537770cb42cc2a
Our analysis is aimed at characterizing the properties of the integrated spectrum of active galactic nuclei (AGNs) such as the ubiquity of the Fe K{\alpha} emission in AGNs and the dependence of the spectral parameters on the X-ray luminosity and red
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ae48acbd5343ec1dc72b838087dd98f2
http://hdl.handle.net/11585/143087
http://hdl.handle.net/11585/143087
Publikováno v:
AIP Conference Proceedings.
We present a study of the properties of obscured Active Galactic Nuclei (AGN) detected in the CDFS 1Ms observation and their host galaxies. We limited the analysis to the MUSIC area, for which deep K-band observations obtained with ISAACatVLT are ava
Autor:
M. P. Ulmer, C. Adami, F. Durret, G. Lima Neto, O. Ilbert, G. Covone, E. Cypriano, W. Mahoney, R. Gavazzi, S. Allam, R. Kron, A. Comastri, L. Angelini, M. Cappi
Publikováno v:
X-RAY ASTRONOMY 2009; PRESENT STATUS, MULTI-WAVELENGTH APPROACH AND FUTURE PERSPECTIVES: Proceedings of the International Conference. AIP Conference Proceedings
X-RAY ASTRONOMY 2009; PRESENT STATUS, MULTI-WAVELENGTH APPROACH AND FUTURE PERSPECTIVES: Proceedings of the International Conference. AIP Conference Proceedings, 0000, à renseigner, Unknown Region. pp.302-303, ⟨10.1063/1.3475242⟩
X-RAY ASTRONOMY 2009; PRESENT STATUS, MULTI-WAVELENGTH APPROACH AND FUTURE PERSPECTIVES: Proceedings of the International Conference. AIP Conference Proceedings, 0000, à renseigner, Unknown Region. pp.302-303, ⟨10.1063/1.3475242⟩
International audience; We present a multi-wavelength study on a z~0.9, Cl 1257+4738. The cluster Cl 1257+4738 was found by comparing a ROSAT image with red ground based images, taken to determine if the red galaxies were young dusty ones or old earl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d41008a2e0d3bd15705dc75e34569f58
http://hdl.handle.net/11588/419893
http://hdl.handle.net/11588/419893
Autor:
Volker Beckmann, S. Soldi, C. Ricci, T. J.-L. Courvoisier, J. Alfonso-Garzón, A. Domingo, J. M. Mas-Hesse, P. Lubiński, A. A. Zdziarski, N. Gehrels, A. Comastri, L. Angelini, M. Cappi
Publikováno v:
X-ray Astronomy 2009; Present Status, Multi-wavelength Approach and Future Perspectives
X-ray Astronomy 2009
X-ray Astronomy 2009, Sep 2009, Bologna, Italy. pp.365-368, ⟨10.1063/1.3475259⟩
X-ray Astronomy 2009
X-ray Astronomy 2009, Sep 2009, Bologna, Italy. pp.365-368, ⟨10.1063/1.3475259⟩
International audience; The INTEGRAL mission provides a large data set for studying the hard X-ray properties of AGN and allows to test the unified scheme for AGN. We present results based on the analysis of 199 AGN. A difference between the Seyfert
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1ca6087c3b67d93e4c78ffb0f4bde137
https://hal.science/hal-00656060
https://hal.science/hal-00656060
Autor:
V. Beckmann, T. J.-L. Courvoisier, N. Gehrels, P. Lubiński, J. Malzac, P. O. Petrucci, C. R. Shrader, S. Soldi, Jéro^me Rodriguez, Phillippe Ferrando
Publikováno v:
AIP Conference Proceedings
SIMBOL-X: FOCUSING ON THE HARD X-RAY UNIVERSE: Proceedings of the 2nd International Simbol-X Symposium
SIMBOL-X: FOCUSING ON THE HARD X-RAY UNIVERSE
SIMBOL-X: FOCUSING ON THE HARD X-RAY UNIVERSE, Dec 2008, Paris Cedex 13, France. pp.141-144, ⟨10.1063/1.3149396⟩
SIMBOL-X: FOCUSING ON THE HARD X-RAY UNIVERSE: Proceedings of the 2nd International Simbol-X Symposium
SIMBOL-X: FOCUSING ON THE HARD X-RAY UNIVERSE
SIMBOL-X: FOCUSING ON THE HARD X-RAY UNIVERSE, Dec 2008, Paris Cedex 13, France. pp.141-144, ⟨10.1063/1.3149396⟩
AGN exhibit complex hard X-ray spectra. Our current understanding is that the emission is dominated by inverse Compton processes which take place in the corona above the accretion disk, and that absorption and reflection in a distant absorber play a