Chemical Evolution of the Stellar and Gaseous Components of Galaxies in Hydrodynamical Cosmological Simulations
We present preliminary results on the effects of mergers on the chemical properties of galactic objects in hierarchical clustering scenarios. We adopt a hydrodynamical chemical code that allows to describe the coupled evolution of dark matter and baryons within a cosmological context. We found that...
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creator | Cora, S. A Tissera, P. B Lambas, D. G Mosconi, M. B |
description | We present preliminary results on the effects of mergers on the chemical
properties of galactic objects in hierarchical clustering scenarios. We adopt a
hydrodynamical chemical code that allows to describe the coupled evolution of
dark matter and baryons within a cosmological context. We found that disk-like
and spheroid-like objects have distinctive metallicity patterns that may be the
result of different evolution. |
doi_str_mv | 10.48550/arxiv.astro-ph/0010462 |
format | Article |
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properties of galactic objects in hierarchical clustering scenarios. We adopt a
hydrodynamical chemical code that allows to describe the coupled evolution of
dark matter and baryons within a cosmological context. We found that disk-like
and spheroid-like objects have distinctive metallicity patterns that may be the
result of different evolution.</description><identifier>DOI: 10.48550/arxiv.astro-ph/0010462</identifier><language>eng</language><subject>Physics - Astrophysics of Galaxies ; Physics - Cosmology and Nongalactic Astrophysics ; Physics - Earth and Planetary Astrophysics ; Physics - High Energy Astrophysical Phenomena ; Physics - Instrumentation and Methods for Astrophysics ; Physics - Solar and Stellar Astrophysics</subject><creationdate>2000-10</creationdate><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,780,885</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/astro-ph/0010462$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.astro-ph/0010462$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Cora, S. A</creatorcontrib><creatorcontrib>Tissera, P. B</creatorcontrib><creatorcontrib>Lambas, D. G</creatorcontrib><creatorcontrib>Mosconi, M. B</creatorcontrib><title>Chemical Evolution of the Stellar and Gaseous Components of Galaxies in Hydrodynamical Cosmological Simulations</title><description>We present preliminary results on the effects of mergers on the chemical
properties of galactic objects in hierarchical clustering scenarios. We adopt a
hydrodynamical chemical code that allows to describe the coupled evolution of
dark matter and baryons within a cosmological context. We found that disk-like
and spheroid-like objects have distinctive metallicity patterns that may be the
result of different evolution.</description><subject>Physics - Astrophysics of Galaxies</subject><subject>Physics - Cosmology and Nongalactic Astrophysics</subject><subject>Physics - Earth and Planetary Astrophysics</subject><subject>Physics - High Energy Astrophysical Phenomena</subject><subject>Physics - Instrumentation and Methods for Astrophysics</subject><subject>Physics - Solar and Stellar Astrophysics</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2000</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNotz71qwzAUhmEtHUraa6iWjE70Z1sai0mTQqBDspsTS6oFsmQsO8R338bJdPjg8MKD0AclGyHznGxhuLnrBtI4xKxvt4RQIgr2imLVms414PHuGv00uhhwtHhsDT6NxnsYMASN95BMnBKuYtfHYMKY7l978HBzJmEX8GHWQ9RzgEetiqmLPv4u4-S6ycO9nd7QiwWfzPvzrtD5a3euDtnxZ_9dfR4zKBXLBJVUU2W5YpxLyXlJZcFKoIRfmM6ZzQUTzb_rolTDgRED1EqjC5NboQjwFVo_sou77gfXwTDXi7_u2_rp53-B2loo</recordid><startdate>20001023</startdate><enddate>20001023</enddate><creator>Cora, S. A</creator><creator>Tissera, P. B</creator><creator>Lambas, D. G</creator><creator>Mosconi, M. B</creator><scope>GOX</scope></search><sort><creationdate>20001023</creationdate><title>Chemical Evolution of the Stellar and Gaseous Components of Galaxies in Hydrodynamical Cosmological Simulations</title><author>Cora, S. A ; Tissera, P. B ; Lambas, D. G ; Mosconi, M. B</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a792-4181d19f392338833718627a103b2d52f5424c550b99c3a20ea1f8ed6e5f490a3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2000</creationdate><topic>Physics - Astrophysics of Galaxies</topic><topic>Physics - Cosmology and Nongalactic Astrophysics</topic><topic>Physics - Earth and Planetary Astrophysics</topic><topic>Physics - High Energy Astrophysical Phenomena</topic><topic>Physics - Instrumentation and Methods for Astrophysics</topic><topic>Physics - Solar and Stellar Astrophysics</topic><toplevel>online_resources</toplevel><creatorcontrib>Cora, S. A</creatorcontrib><creatorcontrib>Tissera, P. B</creatorcontrib><creatorcontrib>Lambas, D. G</creatorcontrib><creatorcontrib>Mosconi, M. B</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Cora, S. A</au><au>Tissera, P. B</au><au>Lambas, D. G</au><au>Mosconi, M. B</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Chemical Evolution of the Stellar and Gaseous Components of Galaxies in Hydrodynamical Cosmological Simulations</atitle><date>2000-10-23</date><risdate>2000</risdate><abstract>We present preliminary results on the effects of mergers on the chemical
properties of galactic objects in hierarchical clustering scenarios. We adopt a
hydrodynamical chemical code that allows to describe the coupled evolution of
dark matter and baryons within a cosmological context. We found that disk-like
and spheroid-like objects have distinctive metallicity patterns that may be the
result of different evolution.</abstract><doi>10.48550/arxiv.astro-ph/0010462</doi><oa>free_for_read</oa></addata></record> |
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subjects | Physics - Astrophysics of Galaxies Physics - Cosmology and Nongalactic Astrophysics Physics - Earth and Planetary Astrophysics Physics - High Energy Astrophysical Phenomena Physics - Instrumentation and Methods for Astrophysics Physics - Solar and Stellar Astrophysics |
title | Chemical Evolution of the Stellar and Gaseous Components of Galaxies in Hydrodynamical Cosmological Simulations |
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