Nitrogen Production in Starburst Galaxies Detected by GALEX
We investigate the production of nitrogen in star forming galaxies with ultraviolet (UV) radiation detected by the Galaxy Evolution Explorer Satellite (GALEX). We use a sample of 8,745 GALEX emission line galaxies matched to the Sloan Digital Sky Survey (SDSS) spectroscopic sample. We derive both ga...
Gespeichert in:
| Veröffentlicht in: | arXiv.org 2007-06 |
|---|---|
| Hauptverfasser: | , , , , , , , , , , , , , , , , , , , , , , , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | |
|---|---|
| container_issue | |
| container_start_page | |
| container_title | arXiv.org |
| container_volume | |
| creator | Mallery, Ryan P Kewley, Lisa Rich, R Michael Salim, Samir Charlot, Stephane Tremonti, Christy Seibert, Mark Small, Todd Wyder, Ted Barlow, Tom A ster, Karl Friedman, Peter G Martin, D Christopher Morrissey, Patrick Neff, Susan G Schiminovich, David Bianchi, Luciana Donas, Jose Heckman, Timothy Young-Wook, Lee Madore, Barry F Milliard, Bruno Szalay, Alex S Welsh, Barry Y Suk Young Yi |
| description | We investigate the production of nitrogen in star forming galaxies with ultraviolet (UV) radiation detected by the Galaxy Evolution Explorer Satellite (GALEX). We use a sample of 8,745 GALEX emission line galaxies matched to the Sloan Digital Sky Survey (SDSS) spectroscopic sample. We derive both gas-phase oxygen and nitrogen abundances for the sample, and apply stellar population synthesis models to derive stellar masses and star formation histories of the galaxies. We compare oxygen abundances derived using three different diagnostics. We derive the specific star formation rates of the galaxies by modeling the 7-band GALEX+SDSS photometry. We find that galaxies that have log SFR/M\(_*\) > -10.0 typically have values of log N/O ~0.05 dex less than galaxies with log SFR/M\(_*\) < -10.0 and similar oxygen abundances. |
| doi_str_mv | 10.48550/arxiv.0706.0238 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest_arxiv</sourceid><recordid>TN_cdi_arxiv_primary_0706_0238</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2089956056</sourcerecordid><originalsourceid>FETCH-LOGICAL-a516-9348a710292cf0d1ddc4403bb9df8e8ddcc228368bb79dea58516d80e467bb263</originalsourceid><addsrcrecordid>eNotj89LwzAcxYMgOObuniTgufPb_GqCpzFnFYoK7uCtJE0qGbOdSSrbf7_OeXo8eO_xPgjd5DBnknO412Hvf-dQgJgDofICTQileSYZIVdoFuMGAIgoCOd0gh5efQr9l-vwe-jt0CTfd9h3-CPpYIYQEy71Vu-9i_jRJdckZ7E54HJRrT6v0WWrt9HN_nWK1k-r9fI5q97Kl-WiyjTPRaYok7rIgSjStGBzaxvGgBqjbCudHG1DiKRCGlMo6zSXY8tKcEwUxhBBp-j2PPsHVu-C_9bhUJ8A6xPgGLg7B3ah_xlcTPWmH0I3XqoJSKW4AC7oERXlUgI</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2089956056</pqid></control><display><type>article</type><title>Nitrogen Production in Starburst Galaxies Detected by GALEX</title><source>arXiv.org</source><source>Free E- Journals</source><creator>Mallery, Ryan P ; Kewley, Lisa ; Rich, R Michael ; Salim, Samir ; Charlot, Stephane ; Tremonti, Christy ; Seibert, Mark ; Small, Todd ; Wyder, Ted ; Barlow, Tom A ; ster, Karl ; Friedman, Peter G ; Martin, D Christopher ; Morrissey, Patrick ; Neff, Susan G ; Schiminovich, David ; Bianchi, Luciana ; Donas, Jose ; Heckman, Timothy ; Young-Wook, Lee ; Madore, Barry F ; Milliard, Bruno ; Szalay, Alex S ; Welsh, Barry Y ; Suk Young Yi</creator><creatorcontrib>Mallery, Ryan P ; Kewley, Lisa ; Rich, R Michael ; Salim, Samir ; Charlot, Stephane ; Tremonti, Christy ; Seibert, Mark ; Small, Todd ; Wyder, Ted ; Barlow, Tom A ; ster, Karl ; Friedman, Peter G ; Martin, D Christopher ; Morrissey, Patrick ; Neff, Susan G ; Schiminovich, David ; Bianchi, Luciana ; Donas, Jose ; Heckman, Timothy ; Young-Wook, Lee ; Madore, Barry F ; Milliard, Bruno ; Szalay, Alex S ; Welsh, Barry Y ; Suk Young Yi</creatorcontrib><description>We investigate the production of nitrogen in star forming galaxies with ultraviolet (UV) radiation detected by the Galaxy Evolution Explorer Satellite (GALEX). We use a sample of 8,745 GALEX emission line galaxies matched to the Sloan Digital Sky Survey (SDSS) spectroscopic sample. We derive both gas-phase oxygen and nitrogen abundances for the sample, and apply stellar population synthesis models to derive stellar masses and star formation histories of the galaxies. We compare oxygen abundances derived using three different diagnostics. We derive the specific star formation rates of the galaxies by modeling the 7-band GALEX+SDSS photometry. We find that galaxies that have log SFR/M\(_*\) > -10.0 typically have values of log N/O ~0.05 dex less than galaxies with log SFR/M\(_*\) < -10.0 and similar oxygen abundances.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.0706.0238</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Astronomical models ; Explorer satellites ; Galactic evolution ; Nitrogen ; Oxygen ; Photometry ; 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 ; Sky surveys (astronomy) ; Star & galaxy formation ; Star formation ; Starburst galaxies ; Stellar evolution</subject><ispartof>arXiv.org, 2007-06</ispartof><rights>Notwithstanding the ProQuest Terms and conditions, you may use this content in accordance with the associated terms available at http://arxiv.org/abs/0706.0238.</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,776,780,881,27902</link.rule.ids><backlink>$$Uhttps://doi.org/10.1086/518833$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.48550/arXiv.0706.0238$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Mallery, Ryan P</creatorcontrib><creatorcontrib>Kewley, Lisa</creatorcontrib><creatorcontrib>Rich, R Michael</creatorcontrib><creatorcontrib>Salim, Samir</creatorcontrib><creatorcontrib>Charlot, Stephane</creatorcontrib><creatorcontrib>Tremonti, Christy</creatorcontrib><creatorcontrib>Seibert, Mark</creatorcontrib><creatorcontrib>Small, Todd</creatorcontrib><creatorcontrib>Wyder, Ted</creatorcontrib><creatorcontrib>Barlow, Tom A</creatorcontrib><creatorcontrib>ster, Karl</creatorcontrib><creatorcontrib>Friedman, Peter G</creatorcontrib><creatorcontrib>Martin, D Christopher</creatorcontrib><creatorcontrib>Morrissey, Patrick</creatorcontrib><creatorcontrib>Neff, Susan G</creatorcontrib><creatorcontrib>Schiminovich, David</creatorcontrib><creatorcontrib>Bianchi, Luciana</creatorcontrib><creatorcontrib>Donas, Jose</creatorcontrib><creatorcontrib>Heckman, Timothy</creatorcontrib><creatorcontrib>Young-Wook, Lee</creatorcontrib><creatorcontrib>Madore, Barry F</creatorcontrib><creatorcontrib>Milliard, Bruno</creatorcontrib><creatorcontrib>Szalay, Alex S</creatorcontrib><creatorcontrib>Welsh, Barry Y</creatorcontrib><creatorcontrib>Suk Young Yi</creatorcontrib><title>Nitrogen Production in Starburst Galaxies Detected by GALEX</title><title>arXiv.org</title><description>We investigate the production of nitrogen in star forming galaxies with ultraviolet (UV) radiation detected by the Galaxy Evolution Explorer Satellite (GALEX). We use a sample of 8,745 GALEX emission line galaxies matched to the Sloan Digital Sky Survey (SDSS) spectroscopic sample. We derive both gas-phase oxygen and nitrogen abundances for the sample, and apply stellar population synthesis models to derive stellar masses and star formation histories of the galaxies. We compare oxygen abundances derived using three different diagnostics. We derive the specific star formation rates of the galaxies by modeling the 7-band GALEX+SDSS photometry. We find that galaxies that have log SFR/M\(_*\) > -10.0 typically have values of log N/O ~0.05 dex less than galaxies with log SFR/M\(_*\) < -10.0 and similar oxygen abundances.</description><subject>Astronomical models</subject><subject>Explorer satellites</subject><subject>Galactic evolution</subject><subject>Nitrogen</subject><subject>Oxygen</subject><subject>Photometry</subject><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><subject>Sky surveys (astronomy)</subject><subject>Star & galaxy formation</subject><subject>Star formation</subject><subject>Starburst galaxies</subject><subject>Stellar evolution</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2007</creationdate><recordtype>article</recordtype><sourceid>BENPR</sourceid><sourceid>GOX</sourceid><recordid>eNotj89LwzAcxYMgOObuniTgufPb_GqCpzFnFYoK7uCtJE0qGbOdSSrbf7_OeXo8eO_xPgjd5DBnknO412Hvf-dQgJgDofICTQileSYZIVdoFuMGAIgoCOd0gh5efQr9l-vwe-jt0CTfd9h3-CPpYIYQEy71Vu-9i_jRJdckZ7E54HJRrT6v0WWrt9HN_nWK1k-r9fI5q97Kl-WiyjTPRaYok7rIgSjStGBzaxvGgBqjbCudHG1DiKRCGlMo6zSXY8tKcEwUxhBBp-j2PPsHVu-C_9bhUJ8A6xPgGLg7B3ah_xlcTPWmH0I3XqoJSKW4AC7oERXlUgI</recordid><startdate>20070629</startdate><enddate>20070629</enddate><creator>Mallery, Ryan P</creator><creator>Kewley, Lisa</creator><creator>Rich, R Michael</creator><creator>Salim, Samir</creator><creator>Charlot, Stephane</creator><creator>Tremonti, Christy</creator><creator>Seibert, Mark</creator><creator>Small, Todd</creator><creator>Wyder, Ted</creator><creator>Barlow, Tom A</creator><creator>ster, Karl</creator><creator>Friedman, Peter G</creator><creator>Martin, D Christopher</creator><creator>Morrissey, Patrick</creator><creator>Neff, Susan G</creator><creator>Schiminovich, David</creator><creator>Bianchi, Luciana</creator><creator>Donas, Jose</creator><creator>Heckman, Timothy</creator><creator>Young-Wook, Lee</creator><creator>Madore, Barry F</creator><creator>Milliard, Bruno</creator><creator>Szalay, Alex S</creator><creator>Welsh, Barry Y</creator><creator>Suk Young Yi</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><scope>GOX</scope></search><sort><creationdate>20070629</creationdate><title>Nitrogen Production in Starburst Galaxies Detected by GALEX</title><author>Mallery, Ryan P ; Kewley, Lisa ; Rich, R Michael ; Salim, Samir ; Charlot, Stephane ; Tremonti, Christy ; Seibert, Mark ; Small, Todd ; Wyder, Ted ; Barlow, Tom A ; ster, Karl ; Friedman, Peter G ; Martin, D Christopher ; Morrissey, Patrick ; Neff, Susan G ; Schiminovich, David ; Bianchi, Luciana ; Donas, Jose ; Heckman, Timothy ; Young-Wook, Lee ; Madore, Barry F ; Milliard, Bruno ; Szalay, Alex S ; Welsh, Barry Y ; Suk Young Yi</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a516-9348a710292cf0d1ddc4403bb9df8e8ddcc228368bb79dea58516d80e467bb263</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2007</creationdate><topic>Astronomical models</topic><topic>Explorer satellites</topic><topic>Galactic evolution</topic><topic>Nitrogen</topic><topic>Oxygen</topic><topic>Photometry</topic><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><topic>Sky surveys (astronomy)</topic><topic>Star & galaxy formation</topic><topic>Star formation</topic><topic>Starburst galaxies</topic><topic>Stellar evolution</topic><toplevel>online_resources</toplevel><creatorcontrib>Mallery, Ryan P</creatorcontrib><creatorcontrib>Kewley, Lisa</creatorcontrib><creatorcontrib>Rich, R Michael</creatorcontrib><creatorcontrib>Salim, Samir</creatorcontrib><creatorcontrib>Charlot, Stephane</creatorcontrib><creatorcontrib>Tremonti, Christy</creatorcontrib><creatorcontrib>Seibert, Mark</creatorcontrib><creatorcontrib>Small, Todd</creatorcontrib><creatorcontrib>Wyder, Ted</creatorcontrib><creatorcontrib>Barlow, Tom A</creatorcontrib><creatorcontrib>ster, Karl</creatorcontrib><creatorcontrib>Friedman, Peter G</creatorcontrib><creatorcontrib>Martin, D Christopher</creatorcontrib><creatorcontrib>Morrissey, Patrick</creatorcontrib><creatorcontrib>Neff, Susan G</creatorcontrib><creatorcontrib>Schiminovich, David</creatorcontrib><creatorcontrib>Bianchi, Luciana</creatorcontrib><creatorcontrib>Donas, Jose</creatorcontrib><creatorcontrib>Heckman, Timothy</creatorcontrib><creatorcontrib>Young-Wook, Lee</creatorcontrib><creatorcontrib>Madore, Barry F</creatorcontrib><creatorcontrib>Milliard, Bruno</creatorcontrib><creatorcontrib>Szalay, Alex S</creatorcontrib><creatorcontrib>Welsh, Barry Y</creatorcontrib><creatorcontrib>Suk Young Yi</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</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>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</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><collection>arXiv.org</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Mallery, Ryan P</au><au>Kewley, Lisa</au><au>Rich, R Michael</au><au>Salim, Samir</au><au>Charlot, Stephane</au><au>Tremonti, Christy</au><au>Seibert, Mark</au><au>Small, Todd</au><au>Wyder, Ted</au><au>Barlow, Tom A</au><au>ster, Karl</au><au>Friedman, Peter G</au><au>Martin, D Christopher</au><au>Morrissey, Patrick</au><au>Neff, Susan G</au><au>Schiminovich, David</au><au>Bianchi, Luciana</au><au>Donas, Jose</au><au>Heckman, Timothy</au><au>Young-Wook, Lee</au><au>Madore, Barry F</au><au>Milliard, Bruno</au><au>Szalay, Alex S</au><au>Welsh, Barry Y</au><au>Suk Young Yi</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Nitrogen Production in Starburst Galaxies Detected by GALEX</atitle><jtitle>arXiv.org</jtitle><date>2007-06-29</date><risdate>2007</risdate><eissn>2331-8422</eissn><abstract>We investigate the production of nitrogen in star forming galaxies with ultraviolet (UV) radiation detected by the Galaxy Evolution Explorer Satellite (GALEX). We use a sample of 8,745 GALEX emission line galaxies matched to the Sloan Digital Sky Survey (SDSS) spectroscopic sample. We derive both gas-phase oxygen and nitrogen abundances for the sample, and apply stellar population synthesis models to derive stellar masses and star formation histories of the galaxies. We compare oxygen abundances derived using three different diagnostics. We derive the specific star formation rates of the galaxies by modeling the 7-band GALEX+SDSS photometry. We find that galaxies that have log SFR/M\(_*\) > -10.0 typically have values of log N/O ~0.05 dex less than galaxies with log SFR/M\(_*\) < -10.0 and similar oxygen abundances.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.0706.0238</doi><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | EISSN: 2331-8422 |
| ispartof | arXiv.org, 2007-06 |
| issn | 2331-8422 |
| language | eng |
| recordid | cdi_arxiv_primary_0706_0238 |
| source | arXiv.org; Free E- Journals |
| subjects | Astronomical models Explorer satellites Galactic evolution Nitrogen Oxygen Photometry 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 Sky surveys (astronomy) Star & galaxy formation Star formation Starburst galaxies Stellar evolution |
| title | Nitrogen Production in Starburst Galaxies Detected by GALEX |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-08T23%3A18%3A33IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_arxiv&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Nitrogen%20Production%20in%20Starburst%20Galaxies%20Detected%20by%20GALEX&rft.jtitle=arXiv.org&rft.au=Mallery,%20Ryan%20P&rft.date=2007-06-29&rft.eissn=2331-8422&rft_id=info:doi/10.48550/arxiv.0706.0238&rft_dat=%3Cproquest_arxiv%3E2089956056%3C/proquest_arxiv%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2089956056&rft_id=info:pmid/&rfr_iscdi=true |