Mass Outflow in Active Galactic Nuclei
- 25 May 2001
- journal article
- Published by American Association for the Advancement of Science (AAAS) in Science
- Vol. 292 (5521) , 1500-1501
Abstract
Active galactic nuclei are powered by accretion onto supermassive black holes. In his Perspective, Crenshaw discusses recent insights into the mass outflow from these nuclei, which provide information about the dynamical forces near an active supermassive black hole.Keywords
This publication has 10 references indexed in Scilit:
- Magnetohydrodynamic Production of Relativistic JetsScience, 2001
- Dynamics of Line‐driven Disk Winds in Active Galactic NucleiThe Astrophysical Journal, 2000
- A Kinematic Model for the Narrow-Line Region in NGC 4151The Astronomical Journal, 2000
- Monsters at the Heart of Galaxy FormationScience, 2000
- Dynamics of Warm Absorbing Gas in Seyfert Galaxies: NGC 5548The Astrophysical Journal, 2000
- Discovery of Narrow X-Ray Absorption Lines from NGC 3783 with the [ITAL]Chandra[/ITAL] High Energy Transmission Grating SpectrometerThe Astrophysical Journal, 2000
- Thomson Thick X-Ray Absorption in a Broad Absorption Line Quasar, PG 0946+301The Astrophysical Journal, 2000
- What Determines the Depth of Broad Absorption Lines? Keck HIRES Observations of BALQSO 1603+3002The Astrophysical Journal, 1999
- The Properties of the Relativistic Iron K-Line in NGC 3516The Astrophysical Journal, 1999
- Nuclear Emission in Spiral Nebulae.The Astrophysical Journal, 1943