| 1. Identity statement | ||||
| Reference Type | Journal Article | |||
| Site | mtc-m21d.sid.inpe.br (namespace prefix: upn:44QHRCS) | |||
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S | |||
| Identifier | QABCDSTQQW/46A62UE | |||
| Repository | urlib.net/www/2022/02.02.11.53 | |||
| Last Update | 2022:02.02.11.53.24 (UTC) simone | |||
| Metadata Repository | urlib.net/www/2022/02.02.11.53.24 | |||
| Metadata Last Update | 2023:01.03.16.46.29 (UTC) administrator | |||
| DOI | 10.1093/mnras/stab3230 | |||
| ISSN | 0035-8711 1365-2966 | |||
| Citation Key | Sá-FreitasGCMBSBDM:2022:CoTrFu | |||
| Title | Quenching, bursting, and galaxy shapes: Colour transformation as a function of morphology  | |||
| Year | 2022 | |||
| Month | Jan. | |||
| Access Date | 2025, Dec. 07 | |||
| Type of Work | journal article | |||
| Secondary Type | PRE PI | |||
| Number of Files | 1 | |||
| Size | 2374 KiB | |||
| 2. Context | ||||
| Author | 1 Sá-Freitas, Camila de 2 Gonçalves, T. S. 3 Carvalho, R. R. de 4 Menéndez-Delmestre, K. 5 Barchi, Paulo Henrique 6 Sampaio, V. M. 7 Basu-Zych, A. 8 Darvish, B. 9 Martin, C. | |||
| ORCID | 1 0000-0002-7288-2925 2 3 4 5 6 0000-0001-6556-637X 7 0000-0001-8525-4920 | |||
| Group | 1 2 3 4 5 COPDT-CGIP-INPE-MCTI-GOV-BR | |||
| Affiliation | 1 Universidade Federal do Rio de Janeiro (UFRJ) 2 Universidade Federal do Rio de Janeiro (UFRJ) 3 Universidade Cruzeiro do Sul 4 Universidade Federal do Rio de Janeiro (UFRJ) 5 Instituto Nacional de Pesquisas Espaciais (INPE) 6 Universidade Cruzeiro do Sul 7 NASA Goddard Space Flight Center 8 California Institute of Technology 9 California Institute of Technology | |||
| Author e-Mail Address | 1 camila.desafreitas@eso.org 2 3 4 5 paulobarchi@gmail.com | |||
| Journal | Monthly Notices of the Royal Astronomical Society | |||
| Volume | 509 | |||
| Number | 3 | |||
| Pages | 3889-3903 | |||
| Secondary Mark | A1_QUÍMICA A1_INTERDISCIPLINAR A1_GEOCIÊNCIAS A1_ENGENHARIAS_III A2_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA A2_ASTRONOMIA_/_FÍSICA B2_ENSINO B5_ENGENHARIAS_IV | |||
| Host Collection | urlib.net/www/2021/06.04.03.40 upn:44QHRCS | |||
| History (UTC) | 2022-02-02 11:53:24 :: simone -> administrator :: 2022-02-02 11:53:25 :: administrator -> simone :: 2022 2022-02-02 11:54:45 :: simone -> administrator :: 2022 2023-01-03 16:46:29 :: administrator -> simone :: 2022 | |||
| 3. Content and structure | ||||
| Is the master or a copy? | is the master | |||
| Content Stage | completed | |||
| Transferable | 1 | |||
| Content Type | External Contribution | |||
| Version Type | publisher | |||
| Keywords | cD galaxies: elliptical and lenticular galaxies: evolution galaxies: spiral galaxies: star formation | |||
| Abstract | Different mechanisms for quenching star formation in galaxies are commonly invoked in the literature, but the relative impact of each one at different cosmic epochs is still unknown. In particular, the relation between these processes and morphological transformation remains poorly understood. In this work, we measure the effectiveness of changes in star formation rates by analysing a new parameter, the Star Formation Acceleration (SFA), as a function of galaxy morphology. This methodology is capable of identifying both bursting and quenching episodes that occurred in the preceding 300 Myr. We use morphological classification catalogues based on Deep Learning techniques. Our final sample has ∼14 200 spirals and ∼2500 ellipticals. We find that elliptical galaxies in the transition region have median shorter quenching time-scales (τ < 1 Gyr) than spirals (τ ≥ 1 Gyr). This result conforms to the scenario in which major mergers and other violent processes play a fundamental role in galaxy evolution for most ellipticals, not only quenching star formation more rapidly but also playing a role in morphological transformation. We also find that ∼two-thirds of galaxies bursting in the green valley in our sample are massive spirals ($M_star ge 10^{11.0}, mathrm{M}_odot$) with signs of disturbance. This is in accordance with the scenario where low-mass galaxies are losing their gas in an interaction with a massive galaxy: while the former is quenching, the last is being refueled and going through a burst, showing signs of recent interaction. | |||
| Area | FISMAT | |||
| Arrangement | urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGIP > Quenching, bursting, and... | |||
| doc Directory Content | access | |||
| source Directory Content | there are no files | |||
| agreement Directory Content |
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| 4. Conditions of access and use | ||||
| data URI | upn:44QHRCS:QABCDSTQQW/46A62UE | |||
| data URL | http://urlib.net/ibi/QABCDSTQQW/46A62UE | |||
| zipped data URL | http://urlib.net/zip/QABCDSTQQW/46A62UE | |||
| Language | en | |||
| Target File | freitas2022_quenching.pdf | |||
| User Group | simone | |||
| Reader Group | administrator simone | |||
| Visibility | shown | |||
| Archiving Policy | allowpublisher allowfinaldraft | |||
| Update Permission | not transferred | |||
| 5. Allied materials | ||||
| Next Higher Units | 8JMKD3MGPCW/46KUES5 | |||
| Citing Item List | sid.inpe.br/bibdigital/2022/04.03.23.11 - 36 | |||
| Dissemination | WEBSCI; PORTALCAPES; MGA; COMPENDEX. | |||
| 6. Notes | ||||
| Empty Fields | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark mirrorrepository nextedition notes parameterlist parentrepositories previousedition previouslowerunit progress project readpermission resumeid rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url | |||
| 7. Description control | ||||
| e-Mail (login) | simone | |||
| update | ||||