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Group connectivity in COSMOS: a tracer of mass assembly history

Group connectivity in COSMOS: a tracer of mass assembly history

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2216559314

Group connectivity in COSMOS: a tracer of mass assembly history

About this item

Full title

Group connectivity in COSMOS: a tracer of mass assembly history

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2019-04

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

More information

Scope and Contents

Contents

Cosmic filaments are the channel through which galaxy groups assemble their mass. Cosmic connectivity, namely the number of filaments connected to a given group, is therefore expected to be an important ingredient in shaping group properties. The local connectivity is measured in COSMOS around X-Ray detected groups between redshift 0.5 and 1.2. To...

Alternative Titles

Full title

Group connectivity in COSMOS: a tracer of mass assembly history

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2216559314

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2216559314

Other Identifiers

E-ISSN

2331-8422

DOI

10.48550/arxiv.1904.11859

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