Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/27229
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Schleicher, Dominik | en_US |
dc.contributor.author | Banerjee, R. | en_US |
dc.contributor.author | Boekholt, T. | en_US |
dc.contributor.author | Bovino, S. | en_US |
dc.contributor.author | Fellhauer, M. | en_US |
dc.contributor.author | GALLI, Daniele | en_US |
dc.contributor.author | Grassi, T. | en_US |
dc.contributor.author | Grete, P. | en_US |
dc.contributor.author | Haugboelle, T. | en_US |
dc.contributor.author | Koertgen, B. | en_US |
dc.contributor.author | Latif, M. | en_US |
dc.contributor.author | Riaz, R. | en_US |
dc.contributor.author | Stutz, A. | en_US |
dc.date.accessioned | 2020-09-09T06:57:07Z | - |
dc.date.available | 2020-09-09T06:57:07Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/27229 | - |
dc.description.abstract | Measuring deuteration fraction in protostellar cores is considered as an important method for age determinations of protostellar cores, and the high deuteration fraction of up to 10% has been considered as evidence for high ages and strong support via magnetic field. In this talk, I will present 3D magneto-hydrodynamical simulations including the deuteration chemistry to explore how the deuteration fraction depends on the dynamical and chemical conditions. I will show that high deuteration fractions can be obtained under a large set of different conditions. | en_US |
dc.language.iso | eng | en_US |
dc.title | Can Deuteration be Used as A Chemical Clock in Protostellar Cores | en_US |
dc.type | Multimedia | - |
dc.identifier.doi | 10.5281/zenodo.808655 | en_US |
dc.identifier.url | https://zenodo.org/record/808655#.X0t0fC-B3-Y | en_US |
dc.relation.medium | ELETTRONICO | en_US |
dc.relation.firstpage | 54 | en_US |
dc.description.numberofauthors | 13 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | DEU | en_US |
dc.contributor.country | CHL | en_US |
dc.contributor.country | DNK | en_US |
dc.relation.ispartofbook | Star Formation from Cores to Clusters | en_US |
dc.type.invited | no | en_US |
dc.relation.conferencename | Star Formation from Cores to Clusters | en_US |
dc.relation.conferenceplace | ESO, Santiago, Cile | en_US |
dc.relation.conferencedate | 6-9 marzo, 2017 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.type.miur | 298 Altro | - |
dc.identifier.adsbibcode | 2017sfcc.confE..54S | 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 | Multimedia | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | O.A. Arcetri | - |
crisitem.author.orcid | 0000-0001-7706-6049 | - |
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File | Descrizione | Dimensioni | Formato | |
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schleicher_2017.pdf | Talk | 2.29 MB | Adobe PDF | Visualizza/apri |
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