Black holes in binaries and galactic nuclei

By L. Kaper, E. V. Heuvel, P. Woudt. 2001

138 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/eaf9106cdf1e9f49859757624621b6fc487fe78b

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1. P. Hopkins
2. Stuart L. Shapiro
3. M. Haehnelt
4. G. Kauffmann
5. M. Elvis
6. M. Shibata
7. E. Gallo
8. M. Volonteri

Citations in the corpus

• A Unified Model for Black Hole X-Ray Binary Jets? (2004, methodology): “The top panel shows data for the GRS 1915+105 plateau reported in detail in Fender et al. (1999); the lower panel the outburst of XTE J1859+226 reported in Brocksopp et al.”
• A Structure for Quasars (2000, background): “Cellotti and Blandford 2000). Even the scale on which these effects occur is not well determined. It is possible then that, e.g. magnetic fields, re-collimate the outflow near the point at which it would otherwise be accelerated radially to BAL velocities, and instead accelerates the flow toward the”
• Collapse of a Rotating Supermassive Star to a Supermassive Black Hole: Fully Relativistic Simulations (2002, background): “Viable stellar dynamical and hydrodynamical routes leading to the formation of SMBHs have been proposed (e.g., Begelman & Rees 1978, Rees 1984, Shapiro & Teukolsky 1985, Quinlan & Shapiro 1990, Rees 1998, 2001; Balberg & Shapiro 2002).”
• The Correlation between black hole mass and bulge velocity dispersion in hierarchical galaxy formation models (2000, background): “It also strengthens theoretical arguments that spheroid formation and the growth of black holes are closely linked (Richstone et al. 1998; Cattaneo, Haehnelt & Rees 1999; Kauffmann & Haehnelt 2000 (KH2000); Monaco, Salucci & Danese 2000; Cavaliere & Vittorini 2000).”
• Radio Sources in Low-Luminosity Active Galactic Nuclei. II. Very Long Baseline Interferometry Detections of Compact Radio Cores and Jets in a Sample of LINERs (2000, unknown): “1999)—many orders of magnitude lower and thus rendering a thermal origin of the radio emission very unlikely. Of course photoelectric absorption could attenuate some of the soft X-ray emission, however, since seven of our galaxies show broad Hα emission (spectral type 1.9) the absorption should only”