===================================================================== ==> in this proposal, more time is being requested for pwesseli.ysoaebe ==> in this proposal, more time is being requested for cwaelken.vegastar ===================================================================== a novel result from iso is the richness of the spectra of the oxygen-rich dust surrounding some stars, in particular young stars the circumstellar disks of which have not yet been dispersed. the new dust features can be attributed to crystalline silicates: the match with laboratory results about such silicates, in particular those from the allende meteorite, is remarkable. the study of these stars may yield clues for the evolution from the amorphous silicates of the interstellar medium to the crystalline ones that are observed in meteorites, comets and interplanetary dust particles. the new emission features essentially all fall in the spectral window (20-80 micron) that has been opened to spectroscopy by iso and that will be closed again for a long time after the end of the mission. the purpose of the present observations is to observe these features with the best achievable accuracy for selected bright objects, in order to construct a database that will be fundamental for the study of the mineralogy of oxygen rich dust.
Instrument
LWS01 , PHT40 , SWS01 , SWS02 , SWS06
Temporal Coverage
1997-01-24T17:00:14Z/1998-04-03T10:41:34Z
Version
1.0
Mission Description
The Infrared Space Observatory (ISO) was the worlds first true orbiting infrared observatory. Equipped with four highly-sophisticated and versatile scientific instruments, it was launched by Ariane in November 1995 and provided astronomers world-wide with a facility of unprecedented sensitivity and capabilities for a detailed exploration of the Universe at infrared wavelengths.
European Space Agency, WAELKENS et al., 1999, 'DETAILED MINERALOGY OF THE OXYGEN-RICH DUST AROUND YOUNG STARS', 1.0, European Space Agency, https://doi.org/10.5270/esa-o7z7580
