===================================================================== ==> in this proposal, more time is being requested for jhron.varlpv ==> this proposal requests an upgrade from priority 3 for jhron.varlpv ===================================================================== variability is a characteristic feature of most agb stars. unfortunately, spectroscopic time series covering many of the r^ant molecular bands and the dust emission simultaneously do not exist. because of the different sensitivity of various observable features to different parameters and components of the atmosphere/envelope of an agb variable (lpv) and because of the strong and time dependent interplay of pulsation, dust and molecules, such simultaneous and homogeneous data are the only way for a complete understanding of the physical processes involved. from the theoretical side, many of the tools for a quantitative interpretation of such complete spectroscopic time series are available now. the sws on board of iso covers the wavelength region where continuous dust emission starts to dominate and most of the important features in the spectra of lpvs (molecular bands of co, sio, h2o, co2, hcn, c2h2 and c3, the solid state features of amorphous and crystalline silicates and sic). while some of the mentioned bands and features can be observed from the ground, this requires different instruments and often excellent observing conditions. other bands accesible with iso are in spectral regions where the earths atmosphere is completely opaque. only iso can provide, probably for a long time, complete, homogeneous and simultaneous data of the molecular features and the dust emission in the atmospheres and envelopes of lpvs. such data are a unique opportunity to test and improve the time dependent models. for the proposal jhron.varlpv time series with sws have been started for four lpvs. however, in view of the many different parameters influencing the time dependent models (c/o ratio, pulsational properties, stellar temperature etc.) a larger set of stars is definitely needed. we therefore propose to extend our ongoing iso programme varlpv.
Instrument
SWS01
Temporal Coverage
1997-01-10T09:06:54Z/1997-10-10T17:43:08Z
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, HRON et al., 1999, 'SPECTRAL VARIABILITY OF LONG PERIOD VARIABLES THE RELATION BETWEEN PULSATION, ATMOSPHERIC STRUCTURE AND DUST FORMATION', 1.0, European Space Agency, https://doi.org/10.5270/esa-m5tys6j
Rights
Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.
