THE ASTROPHYSICS OF GRAVITATIONAL WAVE SOURCES

By J. Centrella. 2003

173 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Ocean Engineering

View Paper: https://www.semanticscholar.org/paper/b63c5694d5d75882e94655a5015f09cb41d06101

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Citations in the corpus

Mass Deficits, Stalling Radii, and the Merger Histories of Elliptical Galaxies (2006, background): “…holes (SBHs) together (Begelman et al. 1980), and binary SBHs are increasingly invoked to explain the properties of normal and active galaxies (Komossa 2003), including active galactic nucleus (AGN) variability (Valtaoja et al. 2000; Xie 2003), the bending and precession of radio jets (Roos…”
The astrophysics of nanohertz gravitational waves (2018, background): “Like with dynamical friction at larger scales, binaries can also stall here, at parsec scales, due to inefficacy of the LC, which is typically known as the “final parsec problem” (Milosavljević and Merritt 2003b, a).”
Ejection of Hypervelocity Stars by the (Binary) Black Hole in the Galactic Center (2003, background): “The existence of BBHs in some galactic centers is a necessary consequence of hierarchical galaxy formation (Begelman, Blandford & Rees 1980; Yu 2002; Milosavljević & Merritt 2002; Volonteri, Haardt & Madau 2002; Komossa 2003)1.”
An Eccentric Circumbinary Accretion Disk and the Detection of Binary Massive Black Holes (2006, background): “Massive binary black holes have only tentatively been identified in astronomical observations (Komossa 2003, 2006; Rodriguez et al. 2006 report evidence for a binary with projected separation of 7.3 pc), but the theoretical case for their existence is very strong.”
The Murmur of the Sleeping Black Hole: Detection of Nuclear Ultraviolet Variability in LINER Galaxies (2005, background): “The observational evidence for the existence of systems of massive black hole pairs has been reviewed recently by Komossa (2003).”
A Compact Supermassive Binary Black Hole System (2006, background): “There is circumstantial evidence thatmost binary black holesmerge in less than a Hubble time (Komossa 2003).”
A Recoiling Supermassive Black Hole in the Quasar SDSS J092712.65+294344.0? (2008, background): “While some of them can be explained by lensing, others very likely represent real pairs (e.g., Kochanek et al. 1999; review by Komossa 2003).3 Is SDSSJ0927+2943 actually a binary quasar 2 http://galex.stsci.edu/GR2/ 3 In this context, it is interesting to mention HE0450-2958, a system consisting of…”