Effects of moderate abundance changes on the atmospheric structure and colours of Mira variables: research note

<i>Aims. <i/>We study the effects of moderate deviations from solar abundances upon the atmospheric structure and colours of typical Mira variables.<i>Methods. <i/>We present two model series of dynamical opacity-sampling models of Mira variables which have (1) 1/3 solar meta...

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Hauptverfasser: Scholz, Michael (VerfasserIn) , Ireland, Michael J. (VerfasserIn) , Wood, Peter R. (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 21 May 2014
In: Astronomy and astrophysics
Year: 2014, Jahrgang: 565
ISSN:1432-0746
DOI:10.1051/0004-6361/201323183
Online-Zugang:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1051/0004-6361/201323183
Verlag, lizenzpflichtig, Volltext: https://www.aanda.org/articles/aa/abs/2014/05/aa23183-13/aa23183-13.html
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Verfasserangaben:M. Scholz, M.J. Ireland, and P.R. Wood

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520 |a <i>Aims. <i/>We study the effects of moderate deviations from solar abundances upon the atmospheric structure and colours of typical Mira variables.<i>Methods. <i/>We present two model series of dynamical opacity-sampling models of Mira variables which have (1) 1/3 solar metallicity; and (2) “mild” S-type C/O abundance ratio ([C/O] = 0.9) with typical Zr enhancement (solar +1.0). These series are compared to a previously studied solar-abundance series which has similar fundamental parameters (mass, luminosity, period, radius) that are close to those of <i>o<i/> Cet.<i>Results. <i/>Both series show noticeable effects of abundance upon stratifications and infrared colours but cycle-to-cycle differences mask these effects at most pulsation phases, with the exception of a narrow-water-filter colour near minimum phase. 
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