Environmental Effects on Gas and Galaxy Evolution in Clusters

The cluster environment is the site of important transformations in galaxies at a relatively recent cosmological epoch: the galactic morphological types and star formation activity have evolved significantly during the last few Gyrs. How is this related to the galactic gas content? The first part of...

Full description

Saved in:
Bibliographic Details
Published in:arXiv.org 2000-09
Main Authors: Poggianti, Bianca M, van Gorkom, Jacqueline H
Format: Article
Language:English
Subjects:
Dependence
Environmental effects
Galactic clusters
Galactic evolution
Galaxies
Red shift
Star & galaxy formation
Star formation
Stellar evolution
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by
cites
container_end_page
container_issue
container_start_page
container_title arXiv.org
container_volume
creator Poggianti, Bianca M
van Gorkom, Jacqueline H
description The cluster environment is the site of important transformations in galaxies at a relatively recent cosmological epoch: the galactic morphological types and star formation activity have evolved significantly during the last few Gyrs. How is this related to the galactic gas content? The first part of this paper briefly presents the optical observations of galaxies in distant clusters, while the second part focuses on the link between the HI content and the star formation activity, presenting the results of a multiwavelength study of the cluster A2670 (z=0.08) where 42 galaxies have been detected in HI. We show the star formation properties of the HI-normal and HI-deficient galaxies and discuss their dependence on the location within the cluster. Finally, we compare A2670 with clusters at intermediate redshift and with the Coma cluster.
format article
fullrecord <record><control><sourceid>proquest</sourceid><recordid>TN_cdi_proquest_journals_2092616580</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2092616580</sourcerecordid><originalsourceid>FETCH-proquest_journals_20926165803</originalsourceid><addsrcrecordid>eNqNyjEKwjAUgOEgCBbtHQLOhfTF1jo4lagHcC9BU0iJL5qXFL29GTyA0z98_4IVIGVddTuAFSuJJiEEtHtoGlmwo8LZBo8Pg1E7rsbR3CJxj_ysiWu85zr9_nA1e5eizWCR9y5RNIE2bDlqR6b8dc22J3XtL9Uz-FcyFIfJp4CZBhAHaOu26YT87_oCYMM3tA</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2092616580</pqid></control><display><type>article</type><title>Environmental Effects on Gas and Galaxy Evolution in Clusters</title><source>Publicly Available Content Database (Proquest) (PQ_SDU_P3)</source><creator>Poggianti, Bianca M ; van Gorkom, Jacqueline H</creator><creatorcontrib>Poggianti, Bianca M ; van Gorkom, Jacqueline H</creatorcontrib><description>The cluster environment is the site of important transformations in galaxies at a relatively recent cosmological epoch: the galactic morphological types and star formation activity have evolved significantly during the last few Gyrs. How is this related to the galactic gas content? The first part of this paper briefly presents the optical observations of galaxies in distant clusters, while the second part focuses on the link between the HI content and the star formation activity, presenting the results of a multiwavelength study of the cluster A2670 (z=0.08) where 42 galaxies have been detected in HI. We show the star formation properties of the HI-normal and HI-deficient galaxies and discuss their dependence on the location within the cluster. Finally, we compare A2670 with clusters at intermediate redshift and with the Coma cluster.</description><identifier>EISSN: 2331-8422</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Dependence ; Environmental effects ; Galactic clusters ; Galactic evolution ; Galaxies ; Red shift ; Star &amp; galaxy formation ; Star formation ; Stellar evolution</subject><ispartof>arXiv.org, 2000-09</ispartof><rights>2000. This work is published under https://arxiv.org/licenses/assumed-1991-2003/license.html (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.proquest.com/docview/2092616580?pq-origsite=primo$$EHTML$$P50$$Gproquest$$Hfree_for_read</linktohtml><link.rule.ids>780,784,25753,37012,44590</link.rule.ids></links><search><creatorcontrib>Poggianti, Bianca M</creatorcontrib><creatorcontrib>van Gorkom, Jacqueline H</creatorcontrib><title>Environmental Effects on Gas and Galaxy Evolution in Clusters</title><title>arXiv.org</title><description>The cluster environment is the site of important transformations in galaxies at a relatively recent cosmological epoch: the galactic morphological types and star formation activity have evolved significantly during the last few Gyrs. How is this related to the galactic gas content? The first part of this paper briefly presents the optical observations of galaxies in distant clusters, while the second part focuses on the link between the HI content and the star formation activity, presenting the results of a multiwavelength study of the cluster A2670 (z=0.08) where 42 galaxies have been detected in HI. We show the star formation properties of the HI-normal and HI-deficient galaxies and discuss their dependence on the location within the cluster. Finally, we compare A2670 with clusters at intermediate redshift and with the Coma cluster.</description><subject>Dependence</subject><subject>Environmental effects</subject><subject>Galactic clusters</subject><subject>Galactic evolution</subject><subject>Galaxies</subject><subject>Red shift</subject><subject>Star &amp; galaxy formation</subject><subject>Star formation</subject><subject>Stellar evolution</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2000</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><recordid>eNqNyjEKwjAUgOEgCBbtHQLOhfTF1jo4lagHcC9BU0iJL5qXFL29GTyA0z98_4IVIGVddTuAFSuJJiEEtHtoGlmwo8LZBo8Pg1E7rsbR3CJxj_ysiWu85zr9_nA1e5eizWCR9y5RNIE2bDlqR6b8dc22J3XtL9Uz-FcyFIfJp4CZBhAHaOu26YT87_oCYMM3tA</recordid><startdate>20000919</startdate><enddate>20000919</enddate><creator>Poggianti, Bianca M</creator><creator>van Gorkom, Jacqueline H</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20000919</creationdate><title>Environmental Effects on Gas and Galaxy Evolution in Clusters</title><author>Poggianti, Bianca M ; van Gorkom, Jacqueline H</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-proquest_journals_20926165803</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2000</creationdate><topic>Dependence</topic><topic>Environmental effects</topic><topic>Galactic clusters</topic><topic>Galactic evolution</topic><topic>Galaxies</topic><topic>Red shift</topic><topic>Star &amp; galaxy formation</topic><topic>Star formation</topic><topic>Stellar evolution</topic><toplevel>online_resources</toplevel><creatorcontrib>Poggianti, Bianca M</creatorcontrib><creatorcontrib>van Gorkom, Jacqueline H</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science &amp; Engineering Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>ProQuest Central Essentials</collection><collection>AUTh Library subscriptions: ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database (Proquest) (PQ_SDU_P3)</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering collection</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Poggianti, Bianca M</au><au>van Gorkom, Jacqueline H</au><format>book</format><genre>document</genre><ristype>GEN</ristype><atitle>Environmental Effects on Gas and Galaxy Evolution in Clusters</atitle><jtitle>arXiv.org</jtitle><date>2000-09-19</date><risdate>2000</risdate><eissn>2331-8422</eissn><abstract>The cluster environment is the site of important transformations in galaxies at a relatively recent cosmological epoch: the galactic morphological types and star formation activity have evolved significantly during the last few Gyrs. How is this related to the galactic gas content? The first part of this paper briefly presents the optical observations of galaxies in distant clusters, while the second part focuses on the link between the HI content and the star formation activity, presenting the results of a multiwavelength study of the cluster A2670 (z=0.08) where 42 galaxies have been detected in HI. We show the star formation properties of the HI-normal and HI-deficient galaxies and discuss their dependence on the location within the cluster. Finally, we compare A2670 with clusters at intermediate redshift and with the Coma cluster.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier EISSN: 2331-8422
ispartof arXiv.org, 2000-09
issn 2331-8422
language eng
recordid cdi_proquest_journals_2092616580
source Publicly Available Content Database (Proquest) (PQ_SDU_P3)
subjects Dependence
Environmental effects
Galactic clusters
Galactic evolution
Galaxies
Red shift
Star & galaxy formation
Star formation
Stellar evolution
title Environmental Effects on Gas and Galaxy Evolution in Clusters
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-29T11%3A39%3A20IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest&rft_val_fmt=info:ofi/fmt:kev:mtx:book&rft.genre=document&rft.atitle=Environmental%20Effects%20on%20Gas%20and%20Galaxy%20Evolution%20in%20Clusters&rft.jtitle=arXiv.org&rft.au=Poggianti,%20Bianca%20M&rft.date=2000-09-19&rft.eissn=2331-8422&rft_id=info:doi/&rft_dat=%3Cproquest%3E2092616580%3C/proquest%3E%3Cgrp_id%3Ecdi_FETCH-proquest_journals_20926165803%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=2092616580&rft_id=info:pmid/&rfr_iscdi=true