Probing the outer atmosphere of carbon stars - C2H2, HCN and C3 features in the SWS range

Details Probing the outer atmosphere of carbon stars - C2H2, HCN and C3 features in the SWS range Probing the outer atmosphere of carbon stars - C2H2, HCN and C3 features in the SWS range

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000esasp.456..315l&link_type=abstract

ISO beyond the peaks: The 2nd ISO workshop on analytical spectroscopy. Eds. A. Salama, M.F.Kessler, K. Leech & B. Schulz. ESA-SP

Computer Science

1

Iso, Stars: Agb And Post-Agb, Stars: Atmospheres, Stars: Variables, Stars: Carbon, Stars: Radiative Transfer

Scientific paper

We have obtained ISO-SWS spectra of a number of carbon-rich AGB stars in the wavelength range 2.4 - 44 μm with a resolution of about 400. We compare these spectra with results of hydrostatic and dynamic model atmospheres. Of special interest are the features which are formed far out in the atmosphere like the C2H2, HCN and C3 features. For these outer regions of the atmosphere deviations from hydrostatic structures are to be expected.

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