NDLI: Circumstellar H2O in M-type AGB stars

Content Provider	Scilit
Author	Maercker, Matthias Schöier, Fredrik L. Olofsson, Hans
Copyright Year	2008
Description	Surprisingly high amounts of $H_{2}$O 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.
Related Links	https://www.cambridge.org/core/services/aop-cambridge-core/content/view/571BEA5E57F51CF43B217628A52709A4/S1743921308021455a.pdf/div-class-title-circumstellar-h-span-class-sub-2-span-o-in-m-type-agb-stars-div.pdf
Ending Page	164
Page Count	2
Starting Page	163
ISSN	17439213
e-ISSN	17439221
DOI	10.1017/s1743921308021455
Journal	Proceedings of the International Astronomical Union
Issue Number	S251
Volume Number	4
Language	English
Publisher	Cambridge University Press (CUP)
Publisher Date	2008-02-01
Access Restriction	Open
Subject Keyword	Proceedings of the International Astronomical Union Astronomy and Astrophysics agb Circumstellar Matter Mass Loss
Content Type	Text
Resource Type	Article
Subject	Astronomy and Astrophysics Space and Planetary Science

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Circumstellar H2O in M-type AGB stars