The optical properties of small spherical iron grains are derived using a Kramers-Kronig-consistent model of the dielectric function including its dependence on temperature and size. Especially discussed is the effect of the size dependence, which results from the limitation of the free path of the free electrons in the metal by the size of the grain, on the absorption behaviour of small iron spheres and spheroids. The estimated absorption properties are applied to study the temperature behaviour of spherical and spheroidal grains which are heated by the interstellar radiation field
Our far infrared studies of both hydrophobic and hydrophilic aerogel grains have demonstrated that t...
The temperature dependence of the surface plasmon resonance in small metal spheres is calculated usi...
Cometary dust is not spherical nor homogeneous, yet these are the assumptions used to model its ther...
The optical properties of small spherical iron grains are derived using a Kramers-Kronig-consistent ...
Interstellar iron in the form of metallic iron nanoparticles may constitute a component of the inter...
We show that the fact that the thermal radiation from small particles follows the Wien law instead o...
The authors used the results of Infrared Astronomy Satellite (IRAS) observations of diffuse medium d...
On a déterminé la probabilité d'absorption sans recul de photons γ par des petites particules de fer...
The optical absorption of small metal particles is investigated using the hard-walled sphere model o...
The absorption spectra of small Ag+_n clusters are calculated at finite vibrational temperature by...
The spectroscopic properties in the FIR-mm range of analogue materials for interstellar refractory g...
Detailed far-infrared (FIR) and mid-infrared (MIR) studies of aluminum small particles have been car...
The temperature dependence of the exchange splitting of the energy bands in ferromagnetic iron has b...
The magneto-optic and optical properties of evaporated and sputtered Ag were studied experimentally ...
Stellar winds are typical features of the AGB evolution. They are formed as the result of the radiat...
Our far infrared studies of both hydrophobic and hydrophilic aerogel grains have demonstrated that t...
The temperature dependence of the surface plasmon resonance in small metal spheres is calculated usi...
Cometary dust is not spherical nor homogeneous, yet these are the assumptions used to model its ther...
The optical properties of small spherical iron grains are derived using a Kramers-Kronig-consistent ...
Interstellar iron in the form of metallic iron nanoparticles may constitute a component of the inter...
We show that the fact that the thermal radiation from small particles follows the Wien law instead o...
The authors used the results of Infrared Astronomy Satellite (IRAS) observations of diffuse medium d...
On a déterminé la probabilité d'absorption sans recul de photons γ par des petites particules de fer...
The optical absorption of small metal particles is investigated using the hard-walled sphere model o...
The absorption spectra of small Ag+_n clusters are calculated at finite vibrational temperature by...
The spectroscopic properties in the FIR-mm range of analogue materials for interstellar refractory g...
Detailed far-infrared (FIR) and mid-infrared (MIR) studies of aluminum small particles have been car...
The temperature dependence of the exchange splitting of the energy bands in ferromagnetic iron has b...
The magneto-optic and optical properties of evaporated and sputtered Ag were studied experimentally ...
Stellar winds are typical features of the AGB evolution. They are formed as the result of the radiat...
Our far infrared studies of both hydrophobic and hydrophilic aerogel grains have demonstrated that t...
The temperature dependence of the surface plasmon resonance in small metal spheres is calculated usi...
Cometary dust is not spherical nor homogeneous, yet these are the assumptions used to model its ther...