Silicate dust particles are an important player in the cosmic life cycle of matter. They have been detected in a wide variety of environments, ranging from nearby protoplanetary disks to distant quasars. This review summarizes the fundamental properties of silicates relevant to astronomical observations and processes. It provides a review of our knowledge about cosmic silicates, mostly based on results from IR spectroscopy
Presolar, circumstellar silicates have been positively identified by their highly anomalous oxygen i...
Many meteorites contain small quantities of microscopic particles with unusual mixes of isotopes. Th...
We discuss ISO spectroscopy of oxygen-rich dust shells surrounding evolved stars. The dust that cond...
Silicates form a major component of cosmic dust. This paper summarizes the main structural and spect...
Abstract. One of the big surprises of the Infrared Space Observatory (ISO) has been the discovery of...
Silicate grains in space have attracted recently a wide interest of astrophysicists due to the i...
Infrared spectroscopy provides a direct handle on the composition and structure of interstellar dust...
The composition of the interstellar silicate dust is investigated. Condensation or alteration of sil...
International audienceSilicate grains in space have attracted recently a wide interest of astrophysi...
are the most abundant solids in disks around growing stars, but presolar silicates have not been fou...
The comparison of interstellar, circumstellar and primitive solar nebula silicates has led to a sign...
Thesis (Ph. D.)--University of Rochester. Department of Physics and Astronomy, 2017.The composition ...
We investigate the composition and shape distribution of silicate dust grains in the interstellar me...
We investigate the IR spectral features of a sample of D-type symbiotic stars in order to constrain ...
We have determined the mineralogical composition of dust in the broad absorption line (BAL) quasar P...
Presolar, circumstellar silicates have been positively identified by their highly anomalous oxygen i...
Many meteorites contain small quantities of microscopic particles with unusual mixes of isotopes. Th...
We discuss ISO spectroscopy of oxygen-rich dust shells surrounding evolved stars. The dust that cond...
Silicates form a major component of cosmic dust. This paper summarizes the main structural and spect...
Abstract. One of the big surprises of the Infrared Space Observatory (ISO) has been the discovery of...
Silicate grains in space have attracted recently a wide interest of astrophysicists due to the i...
Infrared spectroscopy provides a direct handle on the composition and structure of interstellar dust...
The composition of the interstellar silicate dust is investigated. Condensation or alteration of sil...
International audienceSilicate grains in space have attracted recently a wide interest of astrophysi...
are the most abundant solids in disks around growing stars, but presolar silicates have not been fou...
The comparison of interstellar, circumstellar and primitive solar nebula silicates has led to a sign...
Thesis (Ph. D.)--University of Rochester. Department of Physics and Astronomy, 2017.The composition ...
We investigate the composition and shape distribution of silicate dust grains in the interstellar me...
We investigate the IR spectral features of a sample of D-type symbiotic stars in order to constrain ...
We have determined the mineralogical composition of dust in the broad absorption line (BAL) quasar P...
Presolar, circumstellar silicates have been positively identified by their highly anomalous oxygen i...
Many meteorites contain small quantities of microscopic particles with unusual mixes of isotopes. Th...
We discuss ISO spectroscopy of oxygen-rich dust shells surrounding evolved stars. The dust that cond...