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dc.contributor.authorManara, C. F.
dc.contributor.authorNatta, A.
dc.contributor.authorRosotti, G. P.
dc.contributor.authorAlcalá, J. M.
dc.contributor.authorNisini, B.
dc.contributor.authorLodato, G.
dc.contributor.authorTesti, L.
dc.contributor.authorPascucci, I.
dc.contributor.authorHillenbrand, L.
dc.contributor.authorCarpenter, J.
dc.contributor.authorScholz, A.
dc.contributor.authorFedele, D.
dc.contributor.authorFrasca, A.
dc.contributor.authorMulders, G.
dc.contributor.authorRigliaco, E.
dc.contributor.authorScardoni, C.
dc.contributor.authorZari, E.
dc.date.accessioned2020-10-30T16:30:01Z
dc.date.available2020-10-30T16:30:01Z
dc.date.issued2020-07
dc.identifier.citationManara , C F , Natta , A , Rosotti , G P , Alcalá , J M , Nisini , B , Lodato , G , Testi , L , Pascucci , I , Hillenbrand , L , Carpenter , J , Scholz , A , Fedele , D , Frasca , A , Mulders , G , Rigliaco , E , Scardoni , C & Zari , E 2020 , ' X-shooter survey of disk accretion in Upper Scorpius : I. Very high accretion rates at age > 5 Myr ' , Astronomy & Astrophysics , vol. 639 , A58 . https://doi.org/10.1051/0004-6361/202037949en
dc.identifier.issn0004-6361
dc.identifier.otherPURE: 270733304
dc.identifier.otherPURE UUID: e1d3300f-3250-4123-9d97-e85aea210785
dc.identifier.othercrossref: 10.1051/0004-6361/202037949
dc.identifier.otherScopus: 85092017843
dc.identifier.otherWOS: 000550677000005
dc.identifier.urihttp://hdl.handle.net/10023/20865
dc.descriptionFunding: CFM acknowledges an ESO fellowship. This project has received funding from the European Union’s Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie grant agreement No 823823 (DUSTBUSTERS). This work was partly supported by the Deutsche Forschungs-Gemeinschaft (DFG, German Research Foundation) - Ref no. FOR 2634/1 TE 1024/1-1.en
dc.description.abstractDetermining the mechanisms that drive the evolution of protoplanetary disks is a necessary step toward understanding how planets form. For this work, we measured the mass accretion rate for young stellar objects with disks at age > 5 Myr, a critical test for the current models of disk evolution. We present the analysis of the spectra of 36 targets in the ∼5–10 Myr old Upper Scorpius star-forming region for which disk masses were measured with ALMA. We find that the mass accretion rates in this sample of old but still surviving disks are similarly high as those of the younger (∼1−3 Myr old) star-forming regions of Lupus and Chamaeleon I, when considering the dependence on stellar and disk mass. In particular, several disks show high mass accretion rates ≳10−9 M⊙ yr−1 while having low disk masses. Furthermore, the median values of the measured mass accretion rates in the disk mass ranges where our sample is complete at a level ∼60−80% are compatible in these three regions. At the same time, the spread of mass accretion rates at any given disk mass is still > 0.9 dex, even at age > 5 Myr. These results are in contrast with simple models of viscous evolution, which would predict that the values of the mass accretion rate diminish with time, and a tighter correlation with disk mass at age > 5 Myr. Similarly, simple models of internal photoevaporation cannot reproduce the observed mass accretion rates, while external photoevaporation might explain the low disk masses and high accretion rates. A possible partial solution to the discrepancy with the viscous models is that the gas-to-dust ratio of the disks at ∼5–10 Myr is significantly different and higher than the canonical 100, as suggested by some dust and gas disk evolution models. The results shown here require the presence of several interplaying processes, such as detailed dust evolution, external photoevaporation, and possibly MHD winds, to explain the secular evolution of protoplanetary disks.
dc.format.extent18
dc.language.isoeng
dc.relation.ispartofAstronomy & Astrophysicsen
dc.rightsCopyright © 2020 ESO. This work has been made available online in accordance with publisher policies or with permission. Permission for further reuse of this content should be sought from the publisher or the rights holder. This is the author created accepted manuscript following peer review and may differ slightly from the final published version. The final published version of this work is available at https://doi.org/10.1051/0004-6361/202037949 .en
dc.subjectAccredtionen
dc.subjectAccretion disksen
dc.subjectProtoplanetary disksen
dc.subjectStars: pre-main sequenceen
dc.subjectStars: variable: T Taurien
dc.subjectHerbig Ae/Been
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectI-PWen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleX-shooter survey of disk accretion in Upper Scorpius : I. Very high accretion rates at age > 5 Myren
dc.typeJournal articleen
dc.description.versionPostprinten
dc.contributor.institutionUniversity of St Andrews.School of Physics and Astronomyen
dc.contributor.institutionUniversity of St Andrews.St Andrews Centre for Exoplanet Scienceen
dc.identifier.doihttps://doi.org/10.1051/0004-6361/202037949
dc.description.statusPeer revieweden
dc.identifier.urlhttps://arxiv.org/abs/2004.14232en


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