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Modified Newtonian Dynamics Close to Home

descriptionPublicationkeyboard_double_arrow_right Article 26 Oct 2007 English Publisher:American Association for the Advancement of Science (AAAS)Journal:Science, volume 318, pages 568-570 (issn: 0036-8075, eissn: 1095-9203, Copyright policy )
Authors: Christof M. Aegerter;

doi: 10.1126/science.318.5850.568

Modified Newtonian Dynamics Close to Home

Abstract

In his Perspective “Seeing through Dark Matter” (3 August, p. 607), Stacy McGaugh describes the success of a modified Newtonian dynamics (MOND) in explaining the flat rotation curves of galaxies without invoking dark matter. In addition to noting that MOND is in accord with available data and

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selected citations
These citations are derived from selected sources.
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!
1
Average
Average
Average
hybrid