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ZENODO
Conference object . 2018
License: CC BY
Data sources: Datacite
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
ZENODO
Conference object . 2018
License: CC BY
Data sources: ZENODO
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A Lagrangian View On The Relation Between Galaxy And Halo Angular Momentum

Authors: Genel, Shy;

A Lagrangian View On The Relation Between Galaxy And Halo Angular Momentum

Abstract

Observations combined with basic theoretical considerations suggest that disk galaxies have approximately the same specific angular momentum (sAM) as a typical dark matter halo with the corresponding host mass. The most simplistic interpretation of this newly established result is that the baryons that make up the disks have retained the sAM they obtained from cosmological tidal torques throughout their evolution from the intergalactic medium down to the present-day stars within the galaxy. There is evidence, however, that reality may be substantially more complex than this simplistic picture. Here is a theoretical discussion of the sAM of such baryons through various stages in their evolution. It is argued that the sAM evolution during many of these stages is still not well known, is expected to be substantial, and is probably interrelated despite the diversity of scales and physical processes involved. A strong interplay is necessary to obtain a result that mimics the simplistic `retention' picture.

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visibility
download
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!
views
OpenAIRE UsageCountsViews provided by UsageCounts
downloads
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0
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71
30
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