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arxiv: astro-ph/9810378 · v1 · pith:OBDJAWR3new · submitted 1998-10-23 · 🌌 astro-ph

Supermassive Black Holes and the Evolution of Galaxies

classification 🌌 astro-ph
keywords blackgalaxiesholessupermassiveuniversebeencentersclues
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Black holes, an extreme consequence of the mathematics of General Relativity, have long been suspected of being the prime movers of quasars, which emit more energy than any other objects in the Universe. Recent evidence indicates that supermassive black holes, which are probably quasar remnants, reside at the centers of most galaxies. As our knowledge of the demographics of these relics of a violent earlier Universe improve, we see tantalizing clues that they participated intimately in the formation of galaxies and have strongly influenced their present-day structure.

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Cited by 3 Pith papers

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  1. Statistical evidence for massive black hole recoils in active galactic nuclei

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    A statistically significant positive correlation (r ~ 0.12-0.13) exists between the absolute velocity offset of broad Hβ lines and dust reddening in quasars, consistent with a population of recoiling black holes.

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    A neural-network-accelerated hierarchical Bayesian pipeline is developed and validated on a phenomenological model to constrain EMRI population parameters from LISA data.

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    NIRCam-selected AGN hosts split into a 'bridge' group with moderate-to-low SFRs and a 'branch' group above the SFMS with SFR rising with AGN fraction; both populations show recent transitions between star formation an...