In order to study the interaction of light with interstellar grains, the authors represent an irregular particle by a network of interacting dipoles whose polarizability is determined in a first approach by the Clausius-Mossoti relationship. Typically, 10,000 dipoles are considered. In the case of spherical particles, the results from Mie theory are fully recovered. The main interest of this method is to study with good accuracy the implications of surface roughness and/or inhomogeneities on optical properties in the infrared spectral range, particularly of the silicate emission features
In this paper we study the combined effects of size and shape of small solid state particles on the ...
The approach to model composite interstellar dust grains, using the exact solution to the light scat...
There are indications that interstellar and interplanetary dust grains have an inhomogeneous and f...
The implications of the observed relationship between the wavelength dependence of interstellar circ...
We present a model for the diffuse interstellar dust that explains the observed wavelength...
Observations of interstellar extinction and polarization indicate that the interstellar medium consi...
Observations of interstellar extinction and polarization indicate that the interstellar medium consi...
[ACCESS RESTRICTED TO THE UNIVERSITY OF MISSOURI AT AUTHOR'S REQUEST.] It is now well recognized tha...
Interstellar dust was first identified through the extinction that it causes of optical starlight. I...
Artículo de publicación ISIContext. In protoplanetary disks micron-size dust grains coagulate to for...
Context. In protoplanetary disks micron-size dust grains coagulate to form larger structures with co...
In this paper we study the combined effects of size and shape of small solid state particles on the ...
We study the polarization of the UV light within the cavities of interstellar grain aggregates model...
The original publication is available at www.springerlink.com Copyright Springer [Full text of this ...
The observed polarization of starlight is regarded as being due to absorption by interstellar dust. ...
In this paper we study the combined effects of size and shape of small solid state particles on the ...
The approach to model composite interstellar dust grains, using the exact solution to the light scat...
There are indications that interstellar and interplanetary dust grains have an inhomogeneous and f...
The implications of the observed relationship between the wavelength dependence of interstellar circ...
We present a model for the diffuse interstellar dust that explains the observed wavelength...
Observations of interstellar extinction and polarization indicate that the interstellar medium consi...
Observations of interstellar extinction and polarization indicate that the interstellar medium consi...
[ACCESS RESTRICTED TO THE UNIVERSITY OF MISSOURI AT AUTHOR'S REQUEST.] It is now well recognized tha...
Interstellar dust was first identified through the extinction that it causes of optical starlight. I...
Artículo de publicación ISIContext. In protoplanetary disks micron-size dust grains coagulate to for...
Context. In protoplanetary disks micron-size dust grains coagulate to form larger structures with co...
In this paper we study the combined effects of size and shape of small solid state particles on the ...
We study the polarization of the UV light within the cavities of interstellar grain aggregates model...
The original publication is available at www.springerlink.com Copyright Springer [Full text of this ...
The observed polarization of starlight is regarded as being due to absorption by interstellar dust. ...
In this paper we study the combined effects of size and shape of small solid state particles on the ...
The approach to model composite interstellar dust grains, using the exact solution to the light scat...
There are indications that interstellar and interplanetary dust grains have an inhomogeneous and f...