Herschel far-infrared imaging observations have revealed the density structure of the interface between H ii regions and molecular clouds in great detail. In particular, pillars and globules are present in many high-mass star-forming regions, such as the Eagle nebula (M 16) and the Rosette molecular cloud, and understanding their origin will help characterize triggered star formation
International audienceWe present a new model for the formation of dense clumps and pillars around HI...
The radiative feedback of massive stars on molecular clouds creates pillars, globules and other feat...
International audienceContext. The expansion of H ii regions can trigger the formation of stars. An ...
Context. Herschel far-infrared imaging observations have revealed the density structure of the inter...
Context. Herschel far-infrared imaging observations have revealed the density structure of the inter...
Context. Herschel far-infrared imaging observations have revealed the density structure of the inter...
International audienceContext. Herschel far-infrared imaging observations have revealed the density ...
International audienceContext. Herschel far-infrared imaging observations have revealed the density ...
Pillars and globules are present in many high-mass star-forming regions, such as the Eagle nebula (M...
Molecular cloud complexes are structures of molecular gas with sizes up to 50-200 pc. The multi-wave...
International audienceWe present a new model for the formation of dense clumps and pillars around HI...
The radiative feedback of massive stars on molecular clouds creates pillars, globules and other feat...
International audienceContext. The expansion of H ii regions can trigger the formation of stars. An ...
Context. Herschel far-infrared imaging observations have revealed the density structure of the inter...
Context. Herschel far-infrared imaging observations have revealed the density structure of the inter...
Context. Herschel far-infrared imaging observations have revealed the density structure of the inter...
International audienceContext. Herschel far-infrared imaging observations have revealed the density ...
International audienceContext. Herschel far-infrared imaging observations have revealed the density ...
Pillars and globules are present in many high-mass star-forming regions, such as the Eagle nebula (M...
Molecular cloud complexes are structures of molecular gas with sizes up to 50-200 pc. The multi-wave...
International audienceWe present a new model for the formation of dense clumps and pillars around HI...
The radiative feedback of massive stars on molecular clouds creates pillars, globules and other feat...
International audienceContext. The expansion of H ii regions can trigger the formation of stars. An ...