Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/28202
DC Field | Value | Language |
---|---|---|
dc.contributor.author | SPAGNA, Alessandro | en_US |
dc.contributor.author | CURIR, Anna | en_US |
dc.contributor.author | GIAMMARIA, MARCO | en_US |
dc.contributor.author | LATTANZI, Mario Gilberto | en_US |
dc.contributor.author | MURANTE, Giuseppe | en_US |
dc.contributor.author | RE FIORENTIN, Paola | en_US |
dc.date.accessioned | 2020-11-06T15:11:22Z | - |
dc.date.available | 2020-11-06T15:11:22Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.isbn | 9781107170087 | en_US |
dc.identifier.issn | 1743-9213 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/28202 | - |
dc.description.abstract | We have investigated the chemo-dynamical evolution of a Milky Way-like disk galaxy, AqC4, produced by a cosmological simulation integrating a sub-resolution ISM model. We evidence a global inside-out and upside-down disk evolution, that is consistent with a scenario where the ``thin disk'' stars are formed from the accreted gas close to the galactic plane, while the older ``thick disk'' stars are originated in situ at higher heights. Also, the bar appears the most effective heating mechanism in the inner disk. Finally, no significant metallicity-rotation correlation has been observed, in spite of the presence of a negative [Fe/H] radial gradient. | en_US |
dc.language.iso | eng | en_US |
dc.title | Chemo-dynamical signatures in simulated Milky Way-like galaxies | en_US |
dc.type | Conference paper | - |
dc.identifier.doi | 10.1017/S1743921317006019 | en_US |
dc.identifier.isi | 000454738700070 | en_US |
dc.identifier.url | https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/chemodynamical-signatures-in-simulated-milky-waylike-galaxies/3DA716984D646CB6F9511BAE936532EA | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 330 | en_US |
dc.relation.firstpage | 263 | en_US |
dc.type.referee | REF_0 | en_US |
dc.description.international | no | en_US |
dc.contributor.country | ITA | en_US |
dc.relation.alleditors | Recio-Blanco, Alejandra; de Laverny, Patrick; Brown, Anthony G. A.; Prusti, Timo | en_US |
dc.relation.ispartofbook | Astrometry and Astrophysics in the Gaia Sky | en_US |
dc.type.invited | no | en_US |
dc.relation.conferencename | Astrometry and Astrophysics in the Gaia sky | en_US |
dc.relation.conferenceplace | Nice, France | en_US |
dc.relation.conferencedate | 24-28 April, 2017 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.type.miur | 273 Contributo in Atti di convegno | - |
dc.relation.series | PROCEEDINGS OF THE INTERNATIONAL ASTRONOMICAL UNION | en_US |
dc.identifier.adsbibcode | 2018IAUS..330..263S | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Conference paper | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | O.A. Torino | - |
crisitem.author.dept | O.A. Torino | - |
crisitem.author.dept | O.A. Torino | - |
crisitem.author.orcid | 0000-0003-1732-2412 | - |
crisitem.author.orcid | 0000-0003-0429-7748 | - |
crisitem.author.orcid | 0000-0002-4995-0475 | - |
crisitem.journal.journalissn | 1743-9213 | - |
crisitem.journal.ance | E192651 | - |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
Spagna_2018_Proc_IAUS330_p263.pdf | Pdf editoriale | 114.47 kB | Adobe PDF | View/Open |
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