What is the origin of the water vapour signatures in red giant stars?

M. Farzone; N. Ryde; G. M. Harper; J. Lambert; E. Josselin; M. J. Richter; K. Eriksson

doi:10.1051/eas/1360017

What is the origin of the water vapour signatures in red giant stars?

M. Farzone, N. Ryde, G. M. Harper, J. Lambert, E. Josselin, M. J. Richter, K. Eriksson

Research output: Chapter in Book/Report/Conference proceeding › Paper in conference proceeding › peer-review

Abstract

We investigate the occurrence of water vapour signatures in a total of 10 red giants in the solar neighbourhood at mid-infrared wavelengths (12 pm). With the use of high resolution spectra from TEXES and synthesized spectra based on MARCS model atmospheres, we analyse the differences and discuss plausible causes. These include abundance adjustments, the addition of non-photospheric components (MOLspheres) and a different temperature profile.

Original language	English
Title of host publication	EAS Publications Series
Publisher	EDP Sciences
Pages	155-159
Number of pages	5
Volume	60
ISBN (Print)	9782759809974
DOIs	https://doi.org/10.1051/eas/1360017
Publication status	Published - 2013
Event	Betelgeuse Workshop 2012 - The Physics of Red Supergiants: Recent Advances and Open Questions - Paris, France Duration: 2012 Nov 26 → 2012 Nov 29

Publication series

Name	EAS Publications Series
Volume	60
ISSN (Print)	16334760
ISSN (Electronic)	16381963

Conference

Conference	Betelgeuse Workshop 2012 - The Physics of Red Supergiants: Recent Advances and Open Questions
Country/Territory	France
City	Paris
Period	2012/11/26 → 2012/11/29

Subject classification (UKÄ)

Astronomy, Astrophysics and Cosmology

Access to Document

10.1051/eas/1360017

Carl-TryggerStiftelse: Water on Stars
Ryde, N. (PI) & Lambert, J. (Researcher)
2012/01/01 → 2013/12/31
Project: Research

Cite this

@inproceedings{8dbea3dc69a44810a658823a018c7b2e,

title = "What is the origin of the water vapour signatures in red giant stars?",

abstract = "We investigate the occurrence of water vapour signatures in a total of 10 red giants in the solar neighbourhood at mid-infrared wavelengths (12 pm). With the use of high resolution spectra from TEXES and synthesized spectra based on MARCS model atmospheres, we analyse the differences and discuss plausible causes. These include abundance adjustments, the addition of non-photospheric components (MOLspheres) and a different temperature profile.",

author = "M. Farzone and N. Ryde and Harper, {G. M.} and J. Lambert and E. Josselin and Richter, {M. J.} and K. Eriksson",

year = "2013",

doi = "10.1051/eas/1360017",

language = "English",

isbn = "9782759809974",

volume = "60",

series = "EAS Publications Series",

publisher = "EDP Sciences",

pages = "155--159",

booktitle = "EAS Publications Series",

address = "France",

note = "Betelgeuse Workshop 2012 - The Physics of Red Supergiants: Recent Advances and Open Questions ; Conference date: 26-11-2012 Through 29-11-2012",

}

Farzone, M, Ryde, N, Harper, GM, Lambert, J, Josselin, E, Richter, MJ & Eriksson, K 2013, What is the origin of the water vapour signatures in red giant stars? in EAS Publications Series. vol. 60, EAS Publications Series, vol. 60, EDP Sciences, pp. 155-159, Betelgeuse Workshop 2012 - The Physics of Red Supergiants: Recent Advances and Open Questions, Paris, France, 2012/11/26. https://doi.org/10.1051/eas/1360017