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arXiv.org e-Print Archive
Preprint . 1998
Data sources: arXiv.org e-Print Archive
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Oxford University Research Archive
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https://dx.doi.org/10.48550/ar...
Article . 1998
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Supermassive Black Holes and the Evolution of Galaxies

descriptionPublicationkeyboard_double_arrow_right Article , Preprint 01 Jan 1998Embargo end date: 01 Jan 1998 United Kingdom Publisher:arXiv
Authors: Richstone, D; Ajhar, E; Bender, R; Bower, G; Dressler, A; Faber, S; Filippenko, A; +7 Authors

doi: 10.48550/arxiv.astro-ph/9810378

arXiv: http://arxiv.org/abs/astro-ph/9810378

Supermassive Black Holes and the Evolution of Galaxies

Abstract

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.

20 pages, - This is a near-duplicate of the paper in Nature 395, A14, 1998 (Oct 1)

Country
United Kingdom
Related Organizations
Keywords

Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

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    citations
    This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
    		 14
    popularity
    This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
    		 Top 10%
    influence
    This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
    		 Average
    impulse
    This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
14
Top 10%
Average
Average
Green
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