Abstract
The dust samples analysed in this work are laboratory analogues of
silicates and oxides of astronomical interest.
Here, we present the calculated dust extinction cross sections.
The data were acquired using the electron microscope facility located at
the University of Cadiz in Spain. Among the samples, four of them are
natural and six are commercial products. The rest of the silicate
samples are synthesised in the laboratories at the Astrophysikalisches
Institut, Universitats-Stenwarte (AIU), and Osaka University.
(20 data files).
Original language | English |
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Journal | VizieR On-line Data Catalog |
Volume | 364 |
DOIs | |
Publication status | Published - 1 Sept 2020 |
Keywords
- Binaries: X-ray
- Abundances