  We present observations of the embedded massive young stellar object (YSO)
candidate 08576nr292, obtained with X-shooter and SINFONI on the ESO Very Large
Telescope (VLT). The flux-calibrated, medium-resolution X-shooter spectrum (300
- 2500 nm) includes over 300 emission lines, but no (photospheric) absorption
lines and is consistent with a reddened disk spectrum. Among the emission lines
are three hydrogen series and helium lines, both permitted and forbidden metal
lines, and CO first-overtone emission. A representative sample of lines with
different morphologies is presented. The H alpha and Ca II triplet lines are
very strong, with profiles indicative of outflow and - possibly - infall,
usually observed in accreting stars. These lines include a blue-shifted
absorption component at ~ -125 km/s. The He I and metal-line profiles are
double-peaked, with a likely origin in a circumstellar disk. The forbidden
lines, associated with outflow, have a single blue-shifted emission component
centered at -125 km/s, coinciding with the absorption components in H alpha and
Ca II. SINFONI H- and K-band integral-field spectroscopy of the cluster
environment demonstrates that the [Fe II] emission is produced by a jet
originating at the location of 08576nr292. Because the spectral type of the
central object cannot be determined, its mass remains uncertain. We argue that
08576nr292 is an intermediate-mass YSO with a high accretion rate Mdot_acc ~
10^-5 - 10^-6 Msun/yr. These observations demonstrate the potential of
X-shooter and SINFONI to study in great detail an accretion disk-jet system,
rarely seen around the more massive YSOs.
