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arXiv.org e-Print Archive
Preprint . 2005
Data sources: arXiv.org e-Print Archive
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SISSA Digital Library
Conference object . 2004
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https://dx.doi.org/10.48550/ar...
Article . 2005
License: arXiv Non-Exclusive Distribution
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Baryons in Dark Matter Halos

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Conference object 01 Jan 2004Embargo end date: 01 Jan 2005Publisher:arXiv
Authors: Dettmar RJ; Klein U; Salucci, Paolo;

doi: 10.48550/arxiv.astro-ph/0502215

arXiv: http://arxiv.org/abs/astro-ph/0502215

handle: 20.500.11767/15460

Baryons in Dark Matter Halos

Abstract

We present here the preface and the Table of Content of the Proceedings of the Conference "Baryons in Dark Matter Halos" held in Cittanova/Novigrad (HR) on 5-9 October, 2004 and published on-line by PoS (http://pos.sissa.it) which is a new versatile, online proceedings and lecture notes publication service launched by SISSA, Trieste.

6 pages

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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).
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!
0
Average
Average
Average
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