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Cited article:

Circumstellar water vapour in M-type AGB stars: constraints from H$_{\sf 2}$O(1$_{\sf 10}$–1$_{\sf 01}$) lines obtained with Odin

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Circumstellar molecular line emission from S-type AGB stars: mass-loss rates and SiO abundances

S. Ramstedt, F. L. Schöier and H. Olofsson
Astronomy & Astrophysics 499 (2) 515 (2009)
https://doi.org/10.1051/0004-6361/200911730

Circumstellar water vapour in M-type AGB stars: radiative transfer models, abundances, and predictions for HIFI

M. Maercker, F. L. Schöier, H. Olofsson, P. Bergman and S. Ramstedt
Astronomy & Astrophysics 479 (3) 779 (2008)
https://doi.org/10.1051/0004-6361:20078680

The physics and chemistry of circumstellar envelopes of S-stars on the AGB

Sofia Ramstedt, Fredrik L. Schöier and Hans Olofsson
Proceedings of the International Astronomical Union 4 (S251) 167 (2008)
https://doi.org/10.1017/S1743921308021479

Composition and quantities of dust produced by AGB-stars and returned to the interstellar medium

A. S. Ferrarotti and H.-P. Gail
Astronomy & Astrophysics 447 (2) 553 (2006)
https://doi.org/10.1051/0004-6361:20041198

SiO in C-rich circumstellar envelopes of AGB stars: effects of non-LTE chemistry and grain adsorption

F. L. Schöier, H. Olofsson and A. A. Lundgren
Astronomy & Astrophysics 454 (1) 247 (2006)
https://doi.org/10.1051/0004-6361:20054795

The Distribution of SiO in the Circumstellar Envelope around IRC +10216

Fredrik L. Schoier, David Fong, Hans Olofsson, Qizhou Zhang and Nimesh Patel
The Astrophysical Journal 649 (2) 965 (2006)
https://doi.org/10.1086/506199

Circumstellar Atomic Hydrogen in Evolved Stars1

E. Gérard and T. Le Bertre
The Astronomical Journal 132 (6) 2566 (2006)
https://doi.org/10.1086/508811

Observations of the Circumstellar Water \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $1_{10}arrow 1_{01}$ \end{document} and Ammonia \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{! wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $1_{0}arrow 0_{0}$ \end{document} Lines in IRC +10216 by theOdinSatellite

T. I. Hasegawa, S. Kwok, N. Koning, et al.
The Astrophysical Journal 637 (2) 791 (2006)
https://doi.org/10.1086/498561

Atomic hydrogen in asymptotic giant branch circumstellar environments. A case study: X Her

E. Gardan, E. Gérard and T. Le Bertre
Monthly Notices of the Royal Astronomical Society 365 (1) 245 (2006)
https://doi.org/10.1111/j.1365-2966.2005.09709.x

BIMA CO Observation of EP Aquarii: The Semiregular Pulsating Star with a Double‐Component Line Profile

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The Astrophysical Journal 638 (2) 1041 (2006)
https://doi.org/10.1086/498934

Disklike Structure in the Semiregular Pulsating Star X Herculis

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The Astrophysical Journal 620 (2) 943 (2005)
https://doi.org/10.1086/427145

Probing the inner wind of AGB stars: Interferometric observations of SiO millimetre line emission from the oxygen-rich stars R Dor and L2 Pup

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The circumstellar environments of EP Aqr  and Y CVn  probed by the H I emission at 21 cm

T. Le Bertre and E. Gérard
Astronomy & Astrophysics 419 (2) 549 (2004)
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