Dust and molecular shells in asymptotic giant branch stars - Mid-infrared interferometric observations of R Aquilae, R Aquarii, R Hydrae, W Hydrae, and V Hydrae

Free Access

Issue		A&A Volume 545, September 2012


Article Number		A56
Number of page(s)		31
Section		Stellar atmospheres
DOI		https://doi.org/10.1051/0004-6361/201118150
Published online		10 September 2012

Online material

Appendix A: Visibility model fit results for R Aql, R Aqr, R Hya and V Hya

Table A.1

R Aql: circular fully limb-darkened disk (FDD) and circular uniform disk (UD).

Table A.2

R Aqr: circular fully limb-darkened disk (FDD) + circular Gaussian (G) and circular uniform disk (UD) + circular Gaussian (G).

Table A.3

R Hya: circular fully limb-darkened disk (FDD) and circular uniform disk (UD).

Table A.4

V Hya: circular fully limb-darkened disk (FDD) + circular Gaussian (G) and circular fully limb-darkened disk (FDD) + circular uniform ring (R).

Appendix B: Diameter details

Table B.1

Details of the diameter measurements presented in the right hand panels of Figs. 6 and 7.

Appendix C: Observation log

Table C.1

AT stations used in this study (cf. http://www.eso.org/sci/facilities/paranal/telescopes/vlti/configuration/index.html).

Table C.2

Detailed observation logs of R Aql, R Aqr, R Hya, and V Hya.

Table C.2

continued.

© ESO, 2012

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