%0 Journal Article
%T Spatially resolved atomic and molecular emission from the very low-mass star IRS54
%A R. Garcia Lopez
%A A. Caratti o Garatti
%A G. Weigelt
%A B. Nisini
%A S. Antoniucci
%J Physics
%D 2013
%I arXiv
%X Molecular outflows from very low-mass stars (VLMSs) and brown dwarfs (BDs) have been studied very little, and only a few objects have been directly imaged. Using VLT SINFONI K-band observations, we spatially resolved, for the first time, the H2 emission around IRS54, a ~0.1-0.2 Msun Class I source. The molecular emission shows a complex structure delineating a large outflow cavity and an asymmetric molecular jet. In addition, new [FeII] VLT ISAAC observations at 1.644um allowed us to discover the atomic jet counterpart which extends down to the central source. The outflow structure is similar to those found in low-mass Class I young stellar objects (YSOs) and Classical TTauri stars (CTTSs). However, its Lacc/Lbol ratio is very high (~80%), and the derived mass accretion rate is about one order of magnitude higher than in objects with similar mass, pointing to the young nature of the investigated source.
%U http://arxiv.org/abs/1307.0677v1