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Emission line diagnostics for accretion and outflows in young very low-mass stars and brown dwarfs

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dc.contributor.authorStelzer, B.
dc.contributor.authorAlcalá, J. M.
dc.contributor.authorWhelan, E.
dc.contributor.authorScholz, A.
dc.date.accessioned2014-09-18T13:31:01Z
dc.date.available2014-09-18T13:31:01Z
dc.date.issued2014-01-08
dc.identifier.citationStelzer , B , Alcalá , J M , Whelan , E & Scholz , A 2014 , ' Emission line diagnostics for accretion and outflows in young very low-mass stars and brown dwarfs ' , EPJ Web of Conferences , vol. 64 , 08005 . https://doi.org/10.1051/epjconf/20136408005en
dc.identifier.issn2100-014X
dc.identifier.otherPURE: 149292931
dc.identifier.otherPURE UUID: 657b09c1-82fc-4316-af60-a8e3100c1a3f
dc.identifier.otherBibCode: 2014EPJWC..6408005S
dc.identifier.otherScopus: 84893581155
dc.identifier.otherWOS: 000342352600052
dc.identifier.urihttps://hdl.handle.net/10023/5447
dc.description.abstractWe discuss accretion and outflow properties of three very low-mass young stellar objects based on broad-band mid-resolution X-Shooter/VLT spectra. Our targets (FU Tau A, 2M1207-39, and Par-Lup3-4) have spectral types between M5 and M8, ages between 1Myr and ~ 10Myr, and are known to be accreting from previous studies. The final objective of our project is the determination of mass outflow to accretion rate for objects near or within the substellar regime as a probe for the T Tauri phase of brown dwarfs and the investigation of variability in the accretion and outflow processes.
dc.format.extent6
dc.language.isoeng
dc.relation.ispartofEPJ Web of Conferencesen
dc.rights© Owned by the authors, published by EDP Sciences, 2014. This is an Open Access article distributed under the terms of the Creative Commons Attribution License 2.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited (https://creativecommons.org/licenses/by/2.0/uk/).en
dc.subjectQC Physicsen
dc.subject.lccQCen
dc.titleEmission line diagnostics for accretion and outflows in young very low-mass stars and brown dwarfsen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1051/epjconf/20136408005
dc.description.statusPeer revieweden


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