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

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Figure

Table 1. Target properties and X-shooter observing log. Additional data for Par-Lup3-4 is described in Sect
Figure 1. Mass accretion rate for FU Tau A derived from various emission line fluxes and luminosities using newcalibrations from [21], and from the Hthe luminosity-based α 10 % width
Figure 2. Mass accretion rate of 2M 1207-39 measured throughout the last decade with diluminosity (filled circles), modelling of UV excess (filled triangles) and Hlatter one the plotting symbols denote the highest and the lowest values measured in the respec
Figure 3. Results from X-Shooter spectroscopy of Par-Lup3-4: (Left) - Mass accretion rates calculated fromline luminosities with the calibrations of [21] (black symbols) and same measurements corrected for the greyextinction induced by the edge-on disk (re

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