International audienceContext. Dust grains are determinant for setting the chemical, physical, dynamical, and radiative properties of all the media in which they are present. Their influence depends on the grain composition, size, and geometrical structure which vary throughout the life cycle of dust. In particular, grain growth arises in dense molecular clouds and protoplanetary disks as traced by an enhancement of the dust far-IR emissivity and by the effects of cloudshine and coreshine.Aims. Our aim is to investigate the imprint of the grain characteristics on the dust unpolarised optical properties from the visible to the far-IR wavelengths for isolated grains as well as for aggregates.Methods. Using optical constants for both carbonace...
Artículo de publicación ISIContext. In protoplanetary disks micron-size dust grains coagulate to for...
Artículo de publicación ISIContext. In protoplanetary disks micron-size dust grains coagulate to for...
To determine a plausible range of mass extinction efficiencies (MEE) of terrestrial atmospheric dust...
International audienceContext. Dust grains are determinant for setting the chemical, physical, dynam...
International audienceContext. Dust grains are determinant for setting the chemical, physical, dynam...
International audienceContext. Dust grains are determinant for setting the chemical, physical, dynam...
Context. Dust grains are determinant for setting the chemical, physical, dynamical, and radiative pr...
Context. Dust grains are determinant for setting the chemical, physical, dynamical, and radiative pr...
Context. Dust grains are determinant for setting the chemical, physical, dynamical, and radiative pr...
Context. In protoplanetary disks micron-size dust grains coagulate to form larger structures with co...
Context. In protoplanetary disks micron-size dust grains coagulate to form larger structures with co...
Context. Dust grains coagulate to form dust aggregates in protoplanetary disks. Their porosity can b...
Context. Dust grains coagulate to form dust aggregates in protoplanetary disks. Their porosity can b...
Context. Dust grains coagulate to form dust aggregates in protoplanetary disks. Their porosity can b...
Context. Dust grains coagulate to form dust aggregates in protoplanetary disks. Their porosity can b...
Artículo de publicación ISIContext. In protoplanetary disks micron-size dust grains coagulate to for...
Artículo de publicación ISIContext. In protoplanetary disks micron-size dust grains coagulate to for...
To determine a plausible range of mass extinction efficiencies (MEE) of terrestrial atmospheric dust...
International audienceContext. Dust grains are determinant for setting the chemical, physical, dynam...
International audienceContext. Dust grains are determinant for setting the chemical, physical, dynam...
International audienceContext. Dust grains are determinant for setting the chemical, physical, dynam...
Context. Dust grains are determinant for setting the chemical, physical, dynamical, and radiative pr...
Context. Dust grains are determinant for setting the chemical, physical, dynamical, and radiative pr...
Context. Dust grains are determinant for setting the chemical, physical, dynamical, and radiative pr...
Context. In protoplanetary disks micron-size dust grains coagulate to form larger structures with co...
Context. In protoplanetary disks micron-size dust grains coagulate to form larger structures with co...
Context. Dust grains coagulate to form dust aggregates in protoplanetary disks. Their porosity can b...
Context. Dust grains coagulate to form dust aggregates in protoplanetary disks. Their porosity can b...
Context. Dust grains coagulate to form dust aggregates in protoplanetary disks. Their porosity can b...
Context. Dust grains coagulate to form dust aggregates in protoplanetary disks. Their porosity can b...
Artículo de publicación ISIContext. In protoplanetary disks micron-size dust grains coagulate to for...
Artículo de publicación ISIContext. In protoplanetary disks micron-size dust grains coagulate to for...
To determine a plausible range of mass extinction efficiencies (MEE) of terrestrial atmospheric dust...