Detailed Modelling of the Circumstellar Envelope of the S-type AGB Star W Aquilae

Taissa Danilovich; Per Bergman; Kay Justtanont; Robin Lombaert; Matthias Maercker; Hans G. Olofsson; Sofia Ramstedt; Pierre Royer

Detailed Modelling of the Circumstellar Envelope of the S-type AGB Star W Aquilae

Taissa Danilovich, Per Bergman, Kay Justtanont, Robin Lombaert, Matthias Maercker, Hans G. Olofsson, Sofia Ramstedt, Pierre Royer

Research output: Chapter in Book/Report/Conference proceeding › Conference Paper › Research

Abstract

We present new Herschel HIFI (de Graauw et al. 2010) and PACS (Poglitsch et al. 2010) sub-millimeter and far-infrared line observations of several molecular species towards the S-type AGB star W Aql. We use these observations, which probe a wide range of gas temperatures, to constrain the circumstellar properties of W Aql, including mass-loss rate and molecular abundances.

Original language	English
Title of host publication	WHY GALAXIES CARE ABOUT AGB STARS III:
Subtitle of host publication	A CLOSER LOOK IN SPACE AND TIME
Editors	Kerschbaum, Wing, Hron
Publisher	Astronomical Society of the Pacific
Pages	219-220
Number of pages	2
Volume	497
Publication status	Published - 2015
Externally published	Yes

Publication series

Name	ASP Conference Series
Publisher	Astronomical Society of the Pacific
Volume	497

Access to Document

https://aspbooks.org/custom/publications/paper/497-0219.htmlLicence: Unspecified

Cite this

Danilovich, T., Bergman, P., Justtanont, K., Lombaert, R., Maercker, M., Olofsson, H. G., Ramstedt, S., & Royer, P. (2015). Detailed Modelling of the Circumstellar Envelope of the S-type AGB Star W Aquilae. In Kerschbaum, Wing, & Hron (Eds.), WHY GALAXIES CARE ABOUT AGB STARS III: : A CLOSER LOOK IN SPACE AND TIME (Vol. 497, pp. 219-220). (ASP Conference Series; Vol. 497). Astronomical Society of the Pacific. https://aspbooks.org/custom/publications/paper/497-0219.html

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title = "Detailed Modelling of the Circumstellar Envelope of the S-type AGB Star W Aquilae",

abstract = "We present new Herschel HIFI (de Graauw et al. 2010) and PACS (Poglitsch et al. 2010) sub-millimeter and far-infrared line observations of several molecular species towards the S-type AGB star W Aql. We use these observations, which probe a wide range of gas temperatures, to constrain the circumstellar properties of W Aql, including mass-loss rate and molecular abundances.",

author = "Taissa Danilovich and Per Bergman and Kay Justtanont and Robin Lombaert and Matthias Maercker and Olofsson, {Hans G.} and Sofia Ramstedt and Pierre Royer",

year = "2015",

language = "English",

volume = "497",

series = "ASP Conference Series",

publisher = "Astronomical Society of the Pacific",

pages = "219--220",

editor = "Kerschbaum and Wing and Hron",

booktitle = "WHY GALAXIES CARE ABOUT AGB STARS III:",

address = "United States of America",

}

Danilovich, T, Bergman, P, Justtanont, K, Lombaert, R, Maercker, M, Olofsson, HG, Ramstedt, S & Royer, P 2015, Detailed Modelling of the Circumstellar Envelope of the S-type AGB Star W Aquilae. in Kerschbaum, Wing & Hron (eds), WHY GALAXIES CARE ABOUT AGB STARS III: : A CLOSER LOOK IN SPACE AND TIME. vol. 497, ASP Conference Series, vol. 497, Astronomical Society of the Pacific, pp. 219-220. <https://aspbooks.org/custom/publications/paper/497-0219.html>

Detailed Modelling of the Circumstellar Envelope of the S-type AGB Star W Aquilae. / Danilovich, Taissa; Bergman, Per; Justtanont, Kay et al.
WHY GALAXIES CARE ABOUT AGB STARS III: : A CLOSER LOOK IN SPACE AND TIME. ed. / Kerschbaum; Wing; Hron. Vol. 497 Astronomical Society of the Pacific, 2015. p. 219-220 (ASP Conference Series; Vol. 497).

Research output: Chapter in Book/Report/Conference proceeding › Conference Paper › Research

TY - GEN

T1 - Detailed Modelling of the Circumstellar Envelope of the S-type AGB Star W Aquilae

AU - Danilovich, Taissa

AU - Bergman, Per

AU - Justtanont, Kay

AU - Lombaert, Robin

AU - Maercker, Matthias

AU - Olofsson, Hans G.

AU - Ramstedt, Sofia

AU - Royer, Pierre

PY - 2015

Y1 - 2015

N2 - We present new Herschel HIFI (de Graauw et al. 2010) and PACS (Poglitsch et al. 2010) sub-millimeter and far-infrared line observations of several molecular species towards the S-type AGB star W Aql. We use these observations, which probe a wide range of gas temperatures, to constrain the circumstellar properties of W Aql, including mass-loss rate and molecular abundances.

AB - We present new Herschel HIFI (de Graauw et al. 2010) and PACS (Poglitsch et al. 2010) sub-millimeter and far-infrared line observations of several molecular species towards the S-type AGB star W Aql. We use these observations, which probe a wide range of gas temperatures, to constrain the circumstellar properties of W Aql, including mass-loss rate and molecular abundances.

M3 - Conference Paper

VL - 497

T3 - ASP Conference Series

SP - 219

EP - 220

BT - WHY GALAXIES CARE ABOUT AGB STARS III:

A2 - Kerschbaum, null

A2 - Wing, null

A2 - Hron, null

PB - Astronomical Society of the Pacific

ER -