Near IR imaging of Centaurus group dwarf elliptical galaxies
Detailed studies of dwarf galaxies in the Local Group have revealed an amazing diversity in their star formation histories. Young and intermediate-age stellar populations are observed in some gas-poor dwarf ellipticals, like Fornax and Carina, where naively one would have expected to find preferenti...
Gespeichert in:
| Veröffentlicht in: | Proceedings of the International Astronomical Union 2005-03, Vol.1 (C198), p.49-51 |
|---|---|
| Hauptverfasser: | , , , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | 51 |
|---|---|
| container_issue | C198 |
| container_start_page | 49 |
| container_title | Proceedings of the International Astronomical Union |
| container_volume | 1 |
| creator | Rejkuba, M. Jerjen, H. Da Costa, G. Binggeli, B. Zoccali, M. |
| description | Detailed studies of dwarf galaxies in the Local Group have revealed an amazing diversity in their star formation histories. Young and intermediate-age stellar populations are observed in some gas-poor dwarf ellipticals, like Fornax and Carina, where naively one would have expected to find preferentially old stellar populations. There are evidences that the environment might drive the evolution of these galaxies. In order to explore stellar populations in dwarf galaxies in an environment denser than that of the Local Group we have observed 14 dwarf elliptical galaxies in Centaurus group in near-IR $J_s$ and $K_s$ bands. The intrinsic properties of these galaxies, the metallicities and ages of their stellar populations and the presence or absence of bright, intermediate-age AGB stars will be correlated with extrinsic properties like the local galaxy density. Here we summarize our observations, present the sample and show near-IR color-magnitude diagrams and luminosity functions for ESO269-066 and AM1343-452 dwarf galaxies. |
| doi_str_mv | 10.1017/S1743921305003479 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_journals_225194045</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><cupid>10_1017_S1743921305003479</cupid><sourcerecordid>1400554331</sourcerecordid><originalsourceid>FETCH-LOGICAL-c2749-671693dda73e11e54ed43f68a75f3d7d64b69feef287af684070df5759f0b07c3</originalsourceid><addsrcrecordid>eNp1kFtLw0AQhRdRsFZ_gG-L79GZvWS74IsUL4Wi4OU5bLOzISVt4m6D-u9NadEH8WmGw_nOMIexc4RLBDRXL2iUtAIlaACpjD1go62UWSHw8GdHecxOUloCqHwi9YhdP5KLfPbM65Wr6nXF28CntN64PvaJV7HtO-4_XAycmqbuNnXpGl65xn3WlE7ZUXBNorP9HLO3u9vX6UM2f7qfTW_mWSmMslluMLfSe2ckIZJW5JUM-cQZHaQ3PleL3AaiICbGDboCAz5oo22ABZhSjtnFLreL7XtPaVMs2z6uh5OFEBqtAqUHE-5MZWxTihSKLg5Pxa8Codh2VPzpaGDknnGrRax9Rb_J_1Pf6NhnJQ</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>225194045</pqid></control><display><type>article</type><title>Near IR imaging of Centaurus group dwarf elliptical galaxies</title><source>Cambridge University Press Journals Complete</source><creator>Rejkuba, M. ; Jerjen, H. ; Da Costa, G. ; Binggeli, B. ; Zoccali, M.</creator><creatorcontrib>Rejkuba, M. ; Jerjen, H. ; Da Costa, G. ; Binggeli, B. ; Zoccali, M.</creatorcontrib><description>Detailed studies of dwarf galaxies in the Local Group have revealed an amazing diversity in their star formation histories. Young and intermediate-age stellar populations are observed in some gas-poor dwarf ellipticals, like Fornax and Carina, where naively one would have expected to find preferentially old stellar populations. There are evidences that the environment might drive the evolution of these galaxies. In order to explore stellar populations in dwarf galaxies in an environment denser than that of the Local Group we have observed 14 dwarf elliptical galaxies in Centaurus group in near-IR $J_s$ and $K_s$ bands. The intrinsic properties of these galaxies, the metallicities and ages of their stellar populations and the presence or absence of bright, intermediate-age AGB stars will be correlated with extrinsic properties like the local galaxy density. Here we summarize our observations, present the sample and show near-IR color-magnitude diagrams and luminosity functions for ESO269-066 and AM1343-452 dwarf galaxies.</description><identifier>ISSN: 1743-9213</identifier><identifier>EISSN: 1743-9221</identifier><identifier>DOI: 10.1017/S1743921305003479</identifier><language>eng</language><publisher>Cambridge, UK: Cambridge University Press</publisher><subject>Astronomy ; Contributed Papers</subject><ispartof>Proceedings of the International Astronomical Union, 2005-03, Vol.1 (C198), p.49-51</ispartof><rights>2005 International Astronomical Union</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c2749-671693dda73e11e54ed43f68a75f3d7d64b69feef287af684070df5759f0b07c3</citedby></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.cambridge.org/core/product/identifier/S1743921305003479/type/journal_article$$EHTML$$P50$$Gcambridge$$H</linktohtml><link.rule.ids>164,314,776,780,27903,27904,55606</link.rule.ids></links><search><creatorcontrib>Rejkuba, M.</creatorcontrib><creatorcontrib>Jerjen, H.</creatorcontrib><creatorcontrib>Da Costa, G.</creatorcontrib><creatorcontrib>Binggeli, B.</creatorcontrib><creatorcontrib>Zoccali, M.</creatorcontrib><title>Near IR imaging of Centaurus group dwarf elliptical galaxies</title><title>Proceedings of the International Astronomical Union</title><addtitle>Proc. IAU</addtitle><description>Detailed studies of dwarf galaxies in the Local Group have revealed an amazing diversity in their star formation histories. Young and intermediate-age stellar populations are observed in some gas-poor dwarf ellipticals, like Fornax and Carina, where naively one would have expected to find preferentially old stellar populations. There are evidences that the environment might drive the evolution of these galaxies. In order to explore stellar populations in dwarf galaxies in an environment denser than that of the Local Group we have observed 14 dwarf elliptical galaxies in Centaurus group in near-IR $J_s$ and $K_s$ bands. The intrinsic properties of these galaxies, the metallicities and ages of their stellar populations and the presence or absence of bright, intermediate-age AGB stars will be correlated with extrinsic properties like the local galaxy density. Here we summarize our observations, present the sample and show near-IR color-magnitude diagrams and luminosity functions for ESO269-066 and AM1343-452 dwarf galaxies.</description><subject>Astronomy</subject><subject>Contributed Papers</subject><issn>1743-9213</issn><issn>1743-9221</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2005</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GNUQQ</sourceid><recordid>eNp1kFtLw0AQhRdRsFZ_gG-L79GZvWS74IsUL4Wi4OU5bLOzISVt4m6D-u9NadEH8WmGw_nOMIexc4RLBDRXL2iUtAIlaACpjD1go62UWSHw8GdHecxOUloCqHwi9YhdP5KLfPbM65Wr6nXF28CntN64PvaJV7HtO-4_XAycmqbuNnXpGl65xn3WlE7ZUXBNorP9HLO3u9vX6UM2f7qfTW_mWSmMslluMLfSe2ckIZJW5JUM-cQZHaQ3PleL3AaiICbGDboCAz5oo22ABZhSjtnFLreL7XtPaVMs2z6uh5OFEBqtAqUHE-5MZWxTihSKLg5Pxa8Codh2VPzpaGDknnGrRax9Rb_J_1Pf6NhnJQ</recordid><startdate>20050301</startdate><enddate>20050301</enddate><creator>Rejkuba, M.</creator><creator>Jerjen, H.</creator><creator>Da Costa, G.</creator><creator>Binggeli, B.</creator><creator>Zoccali, M.</creator><general>Cambridge University Press</general><scope>AAYXX</scope><scope>CITATION</scope><scope>3V.</scope><scope>7XB</scope><scope>88I</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>8FK</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>GNUQQ</scope><scope>H8D</scope><scope>HCIFZ</scope><scope>L7M</scope><scope>M2P</scope><scope>P5Z</scope><scope>P62</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>Q9U</scope></search><sort><creationdate>20050301</creationdate><title>Near IR imaging of Centaurus group dwarf elliptical galaxies</title><author>Rejkuba, M. ; Jerjen, H. ; Da Costa, G. ; Binggeli, B. ; Zoccali, M.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c2749-671693dda73e11e54ed43f68a75f3d7d64b69feef287af684070df5759f0b07c3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2005</creationdate><topic>Astronomy</topic><topic>Contributed Papers</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Rejkuba, M.</creatorcontrib><creatorcontrib>Jerjen, H.</creatorcontrib><creatorcontrib>Da Costa, G.</creatorcontrib><creatorcontrib>Binggeli, B.</creatorcontrib><creatorcontrib>Zoccali, M.</creatorcontrib><collection>CrossRef</collection><collection>ProQuest Central (Corporate)</collection><collection>ProQuest Central (purchase pre-March 2016)</collection><collection>Science Database (Alumni Edition)</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni) (purchase pre-March 2016)</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>Advanced Technologies & Aerospace Collection</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>ProQuest Central Student</collection><collection>Aerospace Database</collection><collection>SciTech Premium Collection</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Science Database</collection><collection>Advanced Technologies & Aerospace Database</collection><collection>ProQuest Advanced Technologies & Aerospace Collection</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>ProQuest Central Basic</collection><jtitle>Proceedings of the International Astronomical Union</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Rejkuba, M.</au><au>Jerjen, H.</au><au>Da Costa, G.</au><au>Binggeli, B.</au><au>Zoccali, M.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Near IR imaging of Centaurus group dwarf elliptical galaxies</atitle><jtitle>Proceedings of the International Astronomical Union</jtitle><addtitle>Proc. IAU</addtitle><date>2005-03-01</date><risdate>2005</risdate><volume>1</volume><issue>C198</issue><spage>49</spage><epage>51</epage><pages>49-51</pages><issn>1743-9213</issn><eissn>1743-9221</eissn><abstract>Detailed studies of dwarf galaxies in the Local Group have revealed an amazing diversity in their star formation histories. Young and intermediate-age stellar populations are observed in some gas-poor dwarf ellipticals, like Fornax and Carina, where naively one would have expected to find preferentially old stellar populations. There are evidences that the environment might drive the evolution of these galaxies. In order to explore stellar populations in dwarf galaxies in an environment denser than that of the Local Group we have observed 14 dwarf elliptical galaxies in Centaurus group in near-IR $J_s$ and $K_s$ bands. The intrinsic properties of these galaxies, the metallicities and ages of their stellar populations and the presence or absence of bright, intermediate-age AGB stars will be correlated with extrinsic properties like the local galaxy density. Here we summarize our observations, present the sample and show near-IR color-magnitude diagrams and luminosity functions for ESO269-066 and AM1343-452 dwarf galaxies.</abstract><cop>Cambridge, UK</cop><pub>Cambridge University Press</pub><doi>10.1017/S1743921305003479</doi><tpages>3</tpages><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 1743-9213 |
| ispartof | Proceedings of the International Astronomical Union, 2005-03, Vol.1 (C198), p.49-51 |
| issn | 1743-9213 1743-9221 |
| language | eng |
| recordid | cdi_proquest_journals_225194045 |
| source | Cambridge University Press Journals Complete |
| subjects | Astronomy Contributed Papers |
| title | Near IR imaging of Centaurus group dwarf elliptical galaxies |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-26T12%3A37%3A50IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Near%20IR%20imaging%20of%20Centaurus%20group%20dwarf%20elliptical%20galaxies&rft.jtitle=Proceedings%20of%20the%20International%20Astronomical%20Union&rft.au=Rejkuba,%20M.&rft.date=2005-03-01&rft.volume=1&rft.issue=C198&rft.spage=49&rft.epage=51&rft.pages=49-51&rft.issn=1743-9213&rft.eissn=1743-9221&rft_id=info:doi/10.1017/S1743921305003479&rft_dat=%3Cproquest_cross%3E1400554331%3C/proquest_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=225194045&rft_id=info:pmid/&rft_cupid=10_1017_S1743921305003479&rfr_iscdi=true |