Circumstellar H2O in M-type AGB stars

Details Circumstellar H2O in M-type AGB stars Circumstellar H2O in M-type AGB stars

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008iaus..251..163m&link_type=abstract

Organic Matter in Space, Proceedings of the International Astronomical Union, IAU Symposium, Volume 251, p. 163-164

Astronomy and Astrophysics

Astronomy

Stars: Agb And Post-Agb, Circumstellar Matter, Mass Loss

Scientific paper

Surprisingly high amounts of H2O have recently been reported in the circumstellar envelope around the M-type AGB star W Hya. However, substantial uncertainties remain, as the required radiative transfer modelling is difficult due to high optical depths, sub-thermal excitation and the sensitivity to the combined radiation field from the central star and dust grains.

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