Publications

Detailed Information

The Velocity Dispersion Function of Very Massive Galaxy Clusters: Abell 2029 and Coma

DC Field Value Language
dc.contributor.authorSohn, Jubee-
dc.contributor.authorGeller, Margaret J.-
dc.contributor.authorZahid, H. Jabran-
dc.contributor.authorFabricant, Daniel G.-
dc.contributor.authorDiaferio, Antonaldo-
dc.contributor.authorRines, Kenneth J.-
dc.date.accessioned2024-05-03T02:27:32Z-
dc.date.available2024-05-03T02:27:32Z-
dc.date.created2024-05-03-
dc.date.created2024-05-03-
dc.date.issued2017-04-
dc.identifier.citationASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, Vol.229 No.2-
dc.identifier.issn0067-0049-
dc.identifier.urihttps://hdl.handle.net/10371/200758-
dc.description.abstractBased on an extensive redshift survey for galaxy clusters Abell 2029 and Coma, we measure the luminosity functions (LFs) and stellar mass functions (SMFs) for the entire cluster member galaxies. Most importantly, we measure the velocity dispersion functions (VDFs) for quiescent members. The MMT/Hectospec redshift survey for galaxies in A2029 identifies 982 spectroscopic members; for 838 members, we derive the central velocity dispersion from the spectroscopy. Coma is the only other cluster surveyed as densely. The LFs, SMFs, and VDFs for A2029 and Coma are essentially identical. The SMFs of the clusters are consistent with simulations. The A2029 and Coma VDFs for quiescent galaxies have a significantly steeper slope than those of field galaxies for velocity dispersion less than or similar to 100 km s(-1). The cluster VDFs also exceed the field at velocity dispersion greater than or similar to 250 km s(-1). The differences between cluster and field VDFs are potentially important tests of simulations and of the formation of structure in the universe.-
dc.language영어-
dc.publisherIOP PUBLISHING LTD-
dc.titleThe Velocity Dispersion Function of Very Massive Galaxy Clusters: Abell 2029 and Coma-
dc.typeArticle-
dc.identifier.doi10.3847/1538-4365/aa653e-
dc.citation.journaltitleASTROPHYSICAL JOURNAL SUPPLEMENT SERIES-
dc.identifier.wosid000398181000002-
dc.identifier.scopusid2-s2.0-85018376792-
dc.citation.number2-
dc.citation.volume229-
dc.description.isOpenAccessY-
dc.contributor.affiliatedAuthorSohn, Jubee-
dc.type.docTypeArticle-
dc.description.journalClass1-
dc.subject.keywordPlusDIGITAL SKY SURVEY-
dc.subject.keywordPlusDARK-MATTER HALOS-
dc.subject.keywordPlusSPECTROSCOPIC LUMINOSITY FUNCTION-
dc.subject.keywordPlusSTELLAR POPULATION SYNTHESIS-
dc.subject.keywordPlusSTAR-FORMATION HISTORIES-
dc.subject.keywordPlusHIGH-SPECTRAL-RESOLUTION-
dc.subject.keywordPlusFIBER-FED SPECTROGRAPH-
dc.subject.keywordPlusVLT DEEP SURVEY-
dc.subject.keywordPlusREDSHIFT SURVEYS-
dc.subject.keywordPlusLENSING SURVEY-
dc.subject.keywordAuthorgalaxies: clusters: individual (Coma, Abell 2029)-
dc.subject.keywordAuthorgalaxies: distances and redshifts-
dc.subject.keywordAuthorgalaxies: fundamental parameters-
dc.subject.keywordAuthorgalaxies: luminosity function, mass function-
Appears in Collections:
Files in This Item:
There are no files associated with this item.

Related Researcher

  • College of Natural Sciences
  • Department of Physics and Astronomy
Research Area Compact Groups of Galaxies, HectoMAP, Velocity Dispersion Function

Altmetrics

Item View & Download Count

  • mendeley

Items in S-Space are protected by copyright, with all rights reserved, unless otherwise indicated.

Share