  Embedded clusters are groups of stars which have not dispersed yet the
residual of the parental cloud where they were born so getting precise
distances and properties of these groups turns out to be an essential task. We
present results for five embedded clusters: [DBS2003]5, [DBS2003]60,
[DBS2003]98, [DBS2003]116 and [DBS2003]117. Results come from a combination of
deep CCD UBVI photometry suitable to identify blue faint stars and infrared
information from available surveys. In turn photometry was linked with proper
motions and parallaxes from Gaia DR2. Each object was treated in a multi-space
using ASteCA, a code especially designed to perform an automatic data analysis
and aimed at providing the fundamental parameters of star groups, in case they
compose a real entity.
