Water Vapor in AGB Stars

Details Water Vapor in AGB Stars Water Vapor in AGB Stars

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000isass..14...43m&link_type=abstract

The Institute of Space and Astronautical Science Report SP No. 14, p. 43-49.

Astronomy and Astrophysics

Astronomy

Stars: Agb And Post-Agb, Stars: Variables: Mira Variables, Stars: Atmospheres, Infrared: Stars

Scientific paper

Structure of the extended atmosphere in AGB stars has been investigated by analyzing H2O bands in the near-infrared region. Based on simple model analysis, we concluded that the time variation in the H2O bands with the variability phase can be attributed to the variation in the physical structure of the extended atmosphere, possibly caused by the shocks in the inner region. High wavelength/spatial resolution observations are crucial for further investigation of the structure.

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