THE INTERSTELLAR MEDIUM AND FEEDBACK IN THE PROGENITORS OF THE COMPACT PASSIVE GALAXIES AT z ∼ 2
Quenched galaxies at z > 2 are nearly all very compact relative to z ~ 0, suggesting a physical connection between high stellar density and efficient, rapid cessation of star-formation. We present rest-frame UV spectra of Lyman-break galaxies (LBGs) at z ~ 3 selected to be candidate progenitors o...
Gespeichert in:
| Veröffentlicht in: | The Astrophysical journal 2015-02, Vol.800 (1), p.1-22 |
|---|---|
| Hauptverfasser: | , , , , , , , , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | 22 |
|---|---|
| container_issue | 1 |
| container_start_page | 1 |
| container_title | The Astrophysical journal |
| container_volume | 800 |
| creator | Williams, Christina C Giavalisco, Mauro Lee, Bomee Tundo, Elena Mobasher, Bahram Nayyeri, Hooshang Ferguson, Henry C Koekemoer, Anton Trump, Jonathan R Cassata, Paolo |
| description | Quenched galaxies at z > 2 are nearly all very compact relative to z ~ 0, suggesting a physical connection between high stellar density and efficient, rapid cessation of star-formation. We present rest-frame UV spectra of Lyman-break galaxies (LBGs) at z ~ 3 selected to be candidate progenitors of the quenched galaxies at z ~ 2 based on their compact rest-frame-optical sizes and high [sigma[subSFR]]. We compare their UV properties to those of more extended LBGs of similar mass and star-formation rate. We propose that massive, compact galaxies undergo more rapid growth of their stellar mass content, perhaps because the gas accretion mechanisms are different, and quench sooner than normally sized LBGs at these epochs. |
| doi_str_mv | 10.1088/0004-637X/800/1/21 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest_osti_</sourceid><recordid>TN_cdi_osti_scitechconnect_22364238</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1768579367</sourcerecordid><originalsourceid>FETCH-LOGICAL-c256t-7ac25c72fbc24c5922091dbf98d03b0f89758d62ef9d34212cd2993c359781523</originalsourceid><addsrcrecordid>eNqN0b1OwzAQB_AIgUT5eAEmSywsIfY5TuzRpG6JSJuqCYjNap1EFLUNxOkAT8BD8TQ8CQllYGS60-mnk-7-jnNB8DXBnHsYY98NaPjocYw94gE5cAaEUe76lIWHf_pj58Ta596DEANnmd8qFE9zNc9ylSRyjiZqGN9PkJwO0Uip4Y2M7jqAejebp2M1jfN0nqF09DOK0slMRjmaySyLHxQay0Q-xipDMkfv6OvjE8GZc1Qt1rY8_62nzv1I5dGtm6TjOJKJa4AFrRsuumpCqJYGfMMEABakWFaCF5guccVFyHgRQFmJgvpAwBTdBdRQJkJOGNBT53K_t7btSluzakvzZOrttjStBqCBD5R36mqvXpr6dVfaVm9W1pTr9WJb1jurSSgoMArY_wcNOOt4EHYU9tQ0tbVNWemXZrVZNG-aYN0npPuP6z4h3SWkiQZCvwGHeHl6</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1768579367</pqid></control><display><type>article</type><title>THE INTERSTELLAR MEDIUM AND FEEDBACK IN THE PROGENITORS OF THE COMPACT PASSIVE GALAXIES AT z ∼ 2</title><source>Institute of Physics Open Access Journal Titles</source><source>Alma/SFX Local Collection</source><source>EZB Electronic Journals Library</source><creator>Williams, Christina C ; Giavalisco, Mauro ; Lee, Bomee ; Tundo, Elena ; Mobasher, Bahram ; Nayyeri, Hooshang ; Ferguson, Henry C ; Koekemoer, Anton ; Trump, Jonathan R ; Cassata, Paolo</creator><creatorcontrib>Williams, Christina C ; Giavalisco, Mauro ; Lee, Bomee ; Tundo, Elena ; Mobasher, Bahram ; Nayyeri, Hooshang ; Ferguson, Henry C ; Koekemoer, Anton ; Trump, Jonathan R ; Cassata, Paolo</creatorcontrib><description>Quenched galaxies at z > 2 are nearly all very compact relative to z ~ 0, suggesting a physical connection between high stellar density and efficient, rapid cessation of star-formation. We present rest-frame UV spectra of Lyman-break galaxies (LBGs) at z ~ 3 selected to be candidate progenitors of the quenched galaxies at z ~ 2 based on their compact rest-frame-optical sizes and high [sigma[subSFR]]. We compare their UV properties to those of more extended LBGs of similar mass and star-formation rate. We propose that massive, compact galaxies undergo more rapid growth of their stellar mass content, perhaps because the gas accretion mechanisms are different, and quench sooner than normally sized LBGs at these epochs.</description><identifier>ISSN: 1538-4357</identifier><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.1088/0004-637X/800/1/21</identifier><language>eng</language><publisher>United States</publisher><subject>ABSORPTION ; ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ; Compact galaxies ; COMPARATIVE EVALUATIONS ; DENSITY ; GALAXIES ; Interstellar matter ; MASS ; METALLICITY ; PHOTON EMISSION ; Progenitors (astrophysics) ; Quenching (cooling) ; RED SHIFT ; Spectra ; STAR EVOLUTION ; Star formation ; ULTRAVIOLET SPECTRA ; VELOCITY ; WOLF-RAYET STARS</subject><ispartof>The Astrophysical journal, 2015-02, Vol.800 (1), p.1-22</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c256t-7ac25c72fbc24c5922091dbf98d03b0f89758d62ef9d34212cd2993c359781523</citedby><cites>FETCH-LOGICAL-c256t-7ac25c72fbc24c5922091dbf98d03b0f89758d62ef9d34212cd2993c359781523</cites><orcidid>0000-0002-9334-8705 ; 0000-0001-8242-9983 ; 0000-0001-9875-8263 ; 0000-0003-2775-2002 ; 0000-0002-5688-0663 ; 0000-0001-8940-6768 ; 0000-0001-6065-7483 ; 0000-0002-7831-8751 ; 0000-0003-4174-0374 ; 0000-0003-3820-2823</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,776,780,881,27903,27904</link.rule.ids><backlink>$$Uhttps://www.osti.gov/biblio/22364238$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Williams, Christina C</creatorcontrib><creatorcontrib>Giavalisco, Mauro</creatorcontrib><creatorcontrib>Lee, Bomee</creatorcontrib><creatorcontrib>Tundo, Elena</creatorcontrib><creatorcontrib>Mobasher, Bahram</creatorcontrib><creatorcontrib>Nayyeri, Hooshang</creatorcontrib><creatorcontrib>Ferguson, Henry C</creatorcontrib><creatorcontrib>Koekemoer, Anton</creatorcontrib><creatorcontrib>Trump, Jonathan R</creatorcontrib><creatorcontrib>Cassata, Paolo</creatorcontrib><title>THE INTERSTELLAR MEDIUM AND FEEDBACK IN THE PROGENITORS OF THE COMPACT PASSIVE GALAXIES AT z ∼ 2</title><title>The Astrophysical journal</title><description>Quenched galaxies at z > 2 are nearly all very compact relative to z ~ 0, suggesting a physical connection between high stellar density and efficient, rapid cessation of star-formation. We present rest-frame UV spectra of Lyman-break galaxies (LBGs) at z ~ 3 selected to be candidate progenitors of the quenched galaxies at z ~ 2 based on their compact rest-frame-optical sizes and high [sigma[subSFR]]. We compare their UV properties to those of more extended LBGs of similar mass and star-formation rate. We propose that massive, compact galaxies undergo more rapid growth of their stellar mass content, perhaps because the gas accretion mechanisms are different, and quench sooner than normally sized LBGs at these epochs.</description><subject>ABSORPTION</subject><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</subject><subject>Compact galaxies</subject><subject>COMPARATIVE EVALUATIONS</subject><subject>DENSITY</subject><subject>GALAXIES</subject><subject>Interstellar matter</subject><subject>MASS</subject><subject>METALLICITY</subject><subject>PHOTON EMISSION</subject><subject>Progenitors (astrophysics)</subject><subject>Quenching (cooling)</subject><subject>RED SHIFT</subject><subject>Spectra</subject><subject>STAR EVOLUTION</subject><subject>Star formation</subject><subject>ULTRAVIOLET SPECTRA</subject><subject>VELOCITY</subject><subject>WOLF-RAYET STARS</subject><issn>1538-4357</issn><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2015</creationdate><recordtype>article</recordtype><recordid>eNqN0b1OwzAQB_AIgUT5eAEmSywsIfY5TuzRpG6JSJuqCYjNap1EFLUNxOkAT8BD8TQ8CQllYGS60-mnk-7-jnNB8DXBnHsYY98NaPjocYw94gE5cAaEUe76lIWHf_pj58Ta596DEANnmd8qFE9zNc9ylSRyjiZqGN9PkJwO0Uip4Y2M7jqAejebp2M1jfN0nqF09DOK0slMRjmaySyLHxQay0Q-xipDMkfv6OvjE8GZc1Qt1rY8_62nzv1I5dGtm6TjOJKJa4AFrRsuumpCqJYGfMMEABakWFaCF5guccVFyHgRQFmJgvpAwBTdBdRQJkJOGNBT53K_t7btSluzakvzZOrttjStBqCBD5R36mqvXpr6dVfaVm9W1pTr9WJb1jurSSgoMArY_wcNOOt4EHYU9tQ0tbVNWemXZrVZNG-aYN0npPuP6z4h3SWkiQZCvwGHeHl6</recordid><startdate>20150210</startdate><enddate>20150210</enddate><creator>Williams, Christina C</creator><creator>Giavalisco, Mauro</creator><creator>Lee, Bomee</creator><creator>Tundo, Elena</creator><creator>Mobasher, Bahram</creator><creator>Nayyeri, Hooshang</creator><creator>Ferguson, Henry C</creator><creator>Koekemoer, Anton</creator><creator>Trump, Jonathan R</creator><creator>Cassata, Paolo</creator><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>OTOTI</scope><orcidid>https://orcid.org/0000-0002-9334-8705</orcidid><orcidid>https://orcid.org/0000-0001-8242-9983</orcidid><orcidid>https://orcid.org/0000-0001-9875-8263</orcidid><orcidid>https://orcid.org/0000-0003-2775-2002</orcidid><orcidid>https://orcid.org/0000-0002-5688-0663</orcidid><orcidid>https://orcid.org/0000-0001-8940-6768</orcidid><orcidid>https://orcid.org/0000-0001-6065-7483</orcidid><orcidid>https://orcid.org/0000-0002-7831-8751</orcidid><orcidid>https://orcid.org/0000-0003-4174-0374</orcidid><orcidid>https://orcid.org/0000-0003-3820-2823</orcidid></search><sort><creationdate>20150210</creationdate><title>THE INTERSTELLAR MEDIUM AND FEEDBACK IN THE PROGENITORS OF THE COMPACT PASSIVE GALAXIES AT z ∼ 2</title><author>Williams, Christina C ; Giavalisco, Mauro ; Lee, Bomee ; Tundo, Elena ; Mobasher, Bahram ; Nayyeri, Hooshang ; Ferguson, Henry C ; Koekemoer, Anton ; Trump, Jonathan R ; Cassata, Paolo</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c256t-7ac25c72fbc24c5922091dbf98d03b0f89758d62ef9d34212cd2993c359781523</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2015</creationdate><topic>ABSORPTION</topic><topic>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</topic><topic>Compact galaxies</topic><topic>COMPARATIVE EVALUATIONS</topic><topic>DENSITY</topic><topic>GALAXIES</topic><topic>Interstellar matter</topic><topic>MASS</topic><topic>METALLICITY</topic><topic>PHOTON EMISSION</topic><topic>Progenitors (astrophysics)</topic><topic>Quenching (cooling)</topic><topic>RED SHIFT</topic><topic>Spectra</topic><topic>STAR EVOLUTION</topic><topic>Star formation</topic><topic>ULTRAVIOLET SPECTRA</topic><topic>VELOCITY</topic><topic>WOLF-RAYET STARS</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Williams, Christina C</creatorcontrib><creatorcontrib>Giavalisco, Mauro</creatorcontrib><creatorcontrib>Lee, Bomee</creatorcontrib><creatorcontrib>Tundo, Elena</creatorcontrib><creatorcontrib>Mobasher, Bahram</creatorcontrib><creatorcontrib>Nayyeri, Hooshang</creatorcontrib><creatorcontrib>Ferguson, Henry C</creatorcontrib><creatorcontrib>Koekemoer, Anton</creatorcontrib><creatorcontrib>Trump, Jonathan R</creatorcontrib><creatorcontrib>Cassata, Paolo</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>OSTI.GOV</collection><jtitle>The Astrophysical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Williams, Christina C</au><au>Giavalisco, Mauro</au><au>Lee, Bomee</au><au>Tundo, Elena</au><au>Mobasher, Bahram</au><au>Nayyeri, Hooshang</au><au>Ferguson, Henry C</au><au>Koekemoer, Anton</au><au>Trump, Jonathan R</au><au>Cassata, Paolo</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>THE INTERSTELLAR MEDIUM AND FEEDBACK IN THE PROGENITORS OF THE COMPACT PASSIVE GALAXIES AT z ∼ 2</atitle><jtitle>The Astrophysical journal</jtitle><date>2015-02-10</date><risdate>2015</risdate><volume>800</volume><issue>1</issue><spage>1</spage><epage>22</epage><pages>1-22</pages><issn>1538-4357</issn><issn>0004-637X</issn><eissn>1538-4357</eissn><abstract>Quenched galaxies at z > 2 are nearly all very compact relative to z ~ 0, suggesting a physical connection between high stellar density and efficient, rapid cessation of star-formation. We present rest-frame UV spectra of Lyman-break galaxies (LBGs) at z ~ 3 selected to be candidate progenitors of the quenched galaxies at z ~ 2 based on their compact rest-frame-optical sizes and high [sigma[subSFR]]. We compare their UV properties to those of more extended LBGs of similar mass and star-formation rate. We propose that massive, compact galaxies undergo more rapid growth of their stellar mass content, perhaps because the gas accretion mechanisms are different, and quench sooner than normally sized LBGs at these epochs.</abstract><cop>United States</cop><doi>10.1088/0004-637X/800/1/21</doi><tpages>22</tpages><orcidid>https://orcid.org/0000-0002-9334-8705</orcidid><orcidid>https://orcid.org/0000-0001-8242-9983</orcidid><orcidid>https://orcid.org/0000-0001-9875-8263</orcidid><orcidid>https://orcid.org/0000-0003-2775-2002</orcidid><orcidid>https://orcid.org/0000-0002-5688-0663</orcidid><orcidid>https://orcid.org/0000-0001-8940-6768</orcidid><orcidid>https://orcid.org/0000-0001-6065-7483</orcidid><orcidid>https://orcid.org/0000-0002-7831-8751</orcidid><orcidid>https://orcid.org/0000-0003-4174-0374</orcidid><orcidid>https://orcid.org/0000-0003-3820-2823</orcidid></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 1538-4357 |
| ispartof | The Astrophysical journal, 2015-02, Vol.800 (1), p.1-22 |
| issn | 1538-4357 0004-637X 1538-4357 |
| language | eng |
| recordid | cdi_osti_scitechconnect_22364238 |
| source | Institute of Physics Open Access Journal Titles; Alma/SFX Local Collection; EZB Electronic Journals Library |
| subjects | ABSORPTION ASTROPHYSICS, COSMOLOGY AND ASTRONOMY Compact galaxies COMPARATIVE EVALUATIONS DENSITY GALAXIES Interstellar matter MASS METALLICITY PHOTON EMISSION Progenitors (astrophysics) Quenching (cooling) RED SHIFT Spectra STAR EVOLUTION Star formation ULTRAVIOLET SPECTRA VELOCITY WOLF-RAYET STARS |
| title | THE INTERSTELLAR MEDIUM AND FEEDBACK IN THE PROGENITORS OF THE COMPACT PASSIVE GALAXIES AT z ∼ 2 |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-24T18%3A34%3A08IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_osti_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=THE%20INTERSTELLAR%20MEDIUM%20AND%20FEEDBACK%20IN%20THE%20PROGENITORS%20OF%20THE%20COMPACT%20PASSIVE%20GALAXIES%20AT%20z%20%E2%88%BC%202&rft.jtitle=The%20Astrophysical%20journal&rft.au=Williams,%20Christina%20C&rft.date=2015-02-10&rft.volume=800&rft.issue=1&rft.spage=1&rft.epage=22&rft.pages=1-22&rft.issn=1538-4357&rft.eissn=1538-4357&rft_id=info:doi/10.1088/0004-637X/800/1/21&rft_dat=%3Cproquest_osti_%3E1768579367%3C/proquest_osti_%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=1768579367&rft_id=info:pmid/&rfr_iscdi=true |