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1by Raue, Martin, Stawarz, Lukasz, Mazin, Daniel, Colin, Pierre, Hui, Michelle, Beilicke, Matthias, Walker, Craig“... bright and compact emission region, powered by a super-massive black hole (SMBH) and an accretion disk...”
Published 2012
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2by Raue, Martin, Stawarz, Lukasz, Mazin, Daniel, Colin, Pierre, Hui, Michelle, Beilicke, Matthias, Walker, Craig“... bright and compact emission region, powered by a super-massive black hole (SMBH) and an accretion disk...”
Published in Journal of Physics: Conference Series (2012)
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3by Agudo, Ivan, Jorstad, Svetlana G., Marscher, Alan P., Larionov, Valeri M., Gomez, Jose L., Lahteenmaki, Anne, Gurwell, Mark, Smith, Paul S., Wiesemeyer, Helmut, Thum, Clemens, Heidt, Jochen“...287 at >14pc from the central supermassive black hole. We employ data from multi-spectral range (total...”
Published 2011
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4“... rotating black holes can produce the MeV/GeV luminosities up to ~ 1044 erg s-1. The hot-flow model...”
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5“... rotating black holes can produce the MeV/GeV luminosities up to ~ 1044 erg s-1. The hot-flow model...”
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6“... rotating black holes can produce the MeV/GeV luminosities up to ~ 1044 erg s-1. The hot-flow model...”
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Conference Object -
7“... rotating black holes can produce the MeV/GeV luminosities up to ~ 1044 erg s-1. The hot-flow model...”
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Conference Object -
8“... rotating black holes can produce the MeV/GeV luminosities up to ~ 1044 erg s-1. The hot-flow model...”
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Conference Object -
9“... rotating black holes can produce the MeV/GeV luminosities up to ~ 1044 erg s-1. The hot-flow model...”
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Conference Object