Variable Line Profiles Due to Non-Axisymmetric Patterns in an Accretion Disc around a Rotating Black Hole

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概要

• 論文の詳細を見る
• Astronomical Society of Japanの論文
• 2001-04-25

著者

• Karas Vladimir

  Astronomical Institute Academy Of Sciences

• MARTOCCHIA Andrea

  Scuola Internazionale Superiore di Studi Avanzati

• SUBR Ladislav

  Astronomical Institute, Charles University Prague

• Subr Ladislav

  Astronomical Institute Charles University Prague

関連論文

• Doppler Tomography of Relativistic Accretion Disks
• Relativistic Iron Features from X-Ray Illuminated Spots and the Measure of the Black Hole Mass in AGN(Poster)
• Non-Linear Resonance in Nearly Geodesic Motion in Low-Mass X-Ray Binaries
• Advection-Dominated Accretion Flow in the Kerr Metric : Propagation of a Wave Pattern
• Of NBOs and kHz QPOs : a Low-Frequency Modulation in Resonant Oscillations of Relativistic Accretion Disks
• Variable Line Profiles Due to Non-Axisymmetric Patterns in an Accretion Disc around a Rotating Black Hole
• Quasi-Periodic Features Due to Clumps Orbiting around a Black Hole
• Polarization of Light from Warm Clouds above an Accretion Disk : Effects of Strong Gravity near a Black Hole
• Relativistic Iron Features from X-Ray Illuminated Spots and the Measure of the Black Hole Mass in AGN(Poster)

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