International audienceContext. The spatial and dynamical structure of star-forming regions can offer insights into stellar formation patterns. The amount of data from current and upcoming surveys calls for robust and objective procedures for detecting structures in order to statistically analyse the various regions and compare them.Aims. We aim to provide the community with a tool capable of detecting, above random expectations, the small-scale significant structure in star-forming regions that could serve as an imprint of the stellar formation process. The tool makes use of the one-point correlation function to determine an appropriate length scale for ϵ and uses nearest-neighbour statistics to determine a minimum number of points Nmin for...
Context. There are a number of methods that identify stellar sub-structure in star forming regions, ...
International audienceContext. Multiplicity and clustering of young pre-main sequence stars appear a...
International audienceContext. Multiplicity and clustering of young pre-main sequence stars appear a...
International audienceContext. The spatial and dynamical structure of star-forming regions can offer...
International audienceContext. The spatial and dynamical structure of star-forming regions can offer...
International audienceContext. The spatial and dynamical structure of star-forming regions can offer...
International audienceContext. The spatial and dynamical structure of star-forming regions can offer...
Context. The spatial and dynamical structure of star-forming regions can offer insights into stellar...
Context. The spatial and dynamical structure of star-forming regions can offer insights into stellar...
Context. The spatial and dynamical structure of star-forming regions can offer insights into stellar...
Context. The spatial and dynamical structure of star-forming regions can offer insights into stellar...
Spatial distribution of young stellar objects (YSOs) in star forming regions (SFRs) may be used as k...
Spatial distribution of young stellar objects (YSOs) in star forming regions (SFRs) may be used as k...
We construct a catalog of the smallest significant young stellar substructures, that we call NESTs, ...
Context. There are a number of methods that identify stellar sub-structure in star forming regions, ...
Context. There are a number of methods that identify stellar sub-structure in star forming regions, ...
International audienceContext. Multiplicity and clustering of young pre-main sequence stars appear a...
International audienceContext. Multiplicity and clustering of young pre-main sequence stars appear a...
International audienceContext. The spatial and dynamical structure of star-forming regions can offer...
International audienceContext. The spatial and dynamical structure of star-forming regions can offer...
International audienceContext. The spatial and dynamical structure of star-forming regions can offer...
International audienceContext. The spatial and dynamical structure of star-forming regions can offer...
Context. The spatial and dynamical structure of star-forming regions can offer insights into stellar...
Context. The spatial and dynamical structure of star-forming regions can offer insights into stellar...
Context. The spatial and dynamical structure of star-forming regions can offer insights into stellar...
Context. The spatial and dynamical structure of star-forming regions can offer insights into stellar...
Spatial distribution of young stellar objects (YSOs) in star forming regions (SFRs) may be used as k...
Spatial distribution of young stellar objects (YSOs) in star forming regions (SFRs) may be used as k...
We construct a catalog of the smallest significant young stellar substructures, that we call NESTs, ...
Context. There are a number of methods that identify stellar sub-structure in star forming regions, ...
Context. There are a number of methods that identify stellar sub-structure in star forming regions, ...
International audienceContext. Multiplicity and clustering of young pre-main sequence stars appear a...
International audienceContext. Multiplicity and clustering of young pre-main sequence stars appear a...