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The Correlation of Outflow Kinematics with Star Formation Rate. VI. Gas Outflows in AGNs
DC Field | Value | Language |
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dc.contributor.author | Woo, Jong-Hak | - |
dc.contributor.author | Son, Donghoon | - |
dc.contributor.author | Rakshit, Suvendu | - |
dc.date.accessioned | 2023-10-11T01:51:27Z | - |
dc.date.available | 2023-10-11T01:51:27Z | - |
dc.date.created | 2020-10-29 | - |
dc.date.issued | 2020-09 | - |
dc.identifier.citation | Astrophysical Journal, Vol.901 No.1, p. 66 | - |
dc.identifier.issn | 0004-637X | - |
dc.identifier.uri | https://hdl.handle.net/10371/195703 | - |
dc.description.abstract | We investigate the connection between ionized gas outflows and star formation activity using a large sample of type 1 and 2 active galactic nuclei (AGNs) with far-infrared detections or star formation rate (SFR) estimates. The strength of ionized gas outflows, measured by the velocity dispersion and velocity shift of the [Oiii] emission line, clearly shows a correlation with SFR. The connection between specific star formation rate (sSFR) and [Oiii] gas velocity dispersion indicates that AGNs with stronger outflows are hosted by galaxies with higher SFR. Compared with star-forming galaxies in the main sequence, both type 1 and type 2 AGNs show sSFRs similar to that of non-AGN galaxies, indicating no instantaneous AGN feedback, while sSFR is higher (lower) for AGNs with stronger (weaker) outflows than that of main-sequence galaxies. These results are consistent with a delayed AGN feedback scenario. However, it is also possible that a decease/increase of gas fraction may cause the correlation without AGN feedback. | - |
dc.language | 영어 | - |
dc.publisher | University of Chicago Press | - |
dc.title | The Correlation of Outflow Kinematics with Star Formation Rate. VI. Gas Outflows in AGNs | - |
dc.type | Article | - |
dc.identifier.doi | 10.3847/1538-4357/abad97 | - |
dc.citation.journaltitle | Astrophysical Journal | - |
dc.identifier.wosid | 000575198200001 | - |
dc.identifier.scopusid | 2-s2.0-85092632601 | - |
dc.citation.number | 1 | - |
dc.citation.startpage | 66 | - |
dc.citation.volume | 901 | - |
dc.description.isOpenAccess | Y | - |
dc.contributor.affiliatedAuthor | Woo, Jong-Hak | - |
dc.type.docType | Article | - |
dc.description.journalClass | 1 | - |
dc.subject.keywordPlus | ACTIVE GALACTIC NUCLEI | - |
dc.subject.keywordPlus | BLACK-HOLE MASSES | - |
dc.subject.keywordPlus | SCALING RELATIONS | - |
dc.subject.keywordPlus | SDSS GALAXIES | - |
dc.subject.keywordPlus | FEEDBACK | - |
dc.subject.keywordPlus | QUASARS | - |
dc.subject.keywordPlus | LUMINOSITIES | - |
dc.subject.keywordPlus | RATIOS | - |
dc.subject.keywordPlus | IMPACT | - |
dc.subject.keywordPlus | GROWTH | - |
dc.subject.keywordAuthor | AGN host galaxies | - |
dc.subject.keywordAuthor | Galaxy formation | - |
dc.subject.keywordAuthor | Supermassive black holes | - |
dc.subject.keywordAuthor | Star formation | - |
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