Laboratory set-up for studying ices at the MIR and FIR region |
| |
| Authors: | J Cantó R Vilaplana M Domingo |
| |
| Institution: | a Department of Applied Physics, Escuela Politécnica Superior de Alcoy (UPV), 03801 Alcoy (Alicante), Spain
b Department of Applied Physics, E.T.S. Ingeniería Geodésica, Cartográfica y Topográfica (UPV), 46022 Valencia, Spain |
| |
| Abstract: | H2O, CO and CO2 ices are condensed on carbonaceous and silicate dust grains in dense interstellar clouds and circumstellar environments. The presence of these ices is inferred by analysing their infrared (IR) spectra. The upcoming Herschel space observatory (HERSCHEL) and ground-based astronomy project (ALMA) will provide new spectral data in the unexplored far infrared (FIR) and sub-millimetre range. In our laboratory we are developing instrumentation to study ices at IR region. One of the key components of our laboratory is a silicon composite bolometer in our IFS. This detector allows us to obtain spectra with a sensitivity much greater than that obtained with a standard deuterated triglycine sulphate (DTGS) detector working at room temperature and under vacuum conditions. We plan to collect mid infrared (MIR) and FIR spectra of simple ices and their mixtures and compare these with observational data. It is also planned to do a systematic laboratory study of the effects that ultraviolet (UV) photolysis and thermal annealing have on the ice band profiles and their structure. |
| |
| Keywords: | Astrochemistry ISM molecules Laboratory infrared spectroscopy |
| 本文献已被 ScienceDirect 等数据库收录！ |
