Emission line diagnostics for accretion and outflows in young very low-mass stars and brown dwarfs
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We 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.
Stelzer , 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/20136408005
EPJ Web of Conferences
© 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/).