Low temperature MIR to submillimeter mass absorption coefficient of interstellar dust analogues

The cosmic ray experimental simulations performed here ex- tend previous studies at lower ion energies ( Mennella et al. 2011 ), giving insight into the astrophysical impli- cations

Furthermore, there is a need to transform the results of laboratory studies of surface processes (sticking, di ffusion, desorption, energy partition, etc.) to the e fficiency

This radiation is absorbed and scattered in the outer edges of the clouds, while the coreshine comes from the inner dense regions lacking any UV or optical

Generation of plasmas containing nano-sized particles, or more generally, dusty plasmas, can be achieved through different plasma sources; the most frequently ones rely on growth

The MAC calculated with the “as- trosilicates” is shown for a 0.1 µm size grain (black), for a log-normal grain size distribution with a mean diameter of 1 µm for spherical

Before the choice of cometary analogues, systematic studies of the variations of polarization with the physical properties of the dust, such as size, porosity, or albedo

Analysis of Murchison, the most studied carbonaceous chondrite, shows the extensive variety of organics (up of tens of thousands of different molecular species) in meteorites

In order to investigate the molecular species that are formed during the dust analogue production, we have performed in-situ mass spectrometry at position QMS1 in Fig. Once at