Supplementary information
From the following article:
A resolved outflow of matter from a brown dwarf
Emma T. Whelan, Thomas P. Ray, Francesca Bacciotti, Antonella Natta, Leonardo Testi & Sofia Randich
Nature 435, 652-654(2 June 2005)
doi:10.1038/nature03598
Supplementary Discussion
Contains details of the spectro-astrometric technique, the method by which any displacement in the emission lines of p-Oph 102 is measured, and details of Additional ELRs and the critical density for a forbidden line scales with Mjet1/2
Supplementary Figure S1
Continuum fitting and removal, using a long-slit spectrum of a typical young star, with an outflow (in this case DG Tau).
Supplementary Figure S2
Spectro-astrometric plots in the vicinity of the [OI] 
6300 line of p-Oph 102, before (top) and after (bottom) continuum straightening.
Supplementary Figure S3
The [OI] 6300, 6363 ELRs were initially fitted with the night sky (NS) lines still present (left panel).
Supplementary Figure S4
The spectro-astrometric plots for the Li6708 and HeI6678 lines
Supplementary Figure S5
Displacement in the [OI] 6300, 6363, [SII] 6731 and HeI 6678 ELRs, with respect to the continuum measured across a large part of the individual orders.
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