The driving mechanism of mass outflows in Mira variables has not yet been fully understood. Recent progress in optical and infrared interferometric techniques has been contributing to studies of the region between the top of the photosphere and the innermost region of the circumstellar dust shell, exactly where mass outflows are expected to be initiated. Infrared interferometric observations of oxygen-rich Mira stars have spatially resolved dense, warm (∼1000–2000 K) molecular layers consisting of H2O, SiO, and CO and extending to ∼2–3 R ⋆ (e.g., Mennesson et al. 1; Perrin et al. 6; Ohnaka et al. 4). The optically thick emission from the warm molecular layers affect the apparent size of Mira stars: the object appears larger than the star itself at wavelengths where the opacities of the above molecular species are higher. In particular, H2O has strong spectral features in the mid-infrared, which causes the angular size to increase from the near-infrared to the mid-infrared as observed toward oxygen-rich Miras.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
B. Mennesson, G. Perrin, G. Chagnon et al., Astrophys. J. 579, 446 (2002)
W. Nowotny, B. Aringer, S. Höfner, R. Gautschy-Loidl, W. Windsteig, Astron. Astrophys. 437, 273 (2005a)
W. Nowotny, T. Lebzelter, J. Hron, S. Höfner, Astron. Astrophys. 437, 285 (2005b)
K. Ohnaka, J. Bergeat, T. Driebe et al., Astron. Astrophys. 429, 1057 (2005)
K. Ohnaka, T. Driebe, G. Weigelt, M. Wittkowski, Astron. Astrophys. 466, 1099 (2007)
G. Perrin, S.T. Ridgway, B. Mennesson et al., Astron. Astrophys. 426, 279 (2004)
R.G. Petrov, F. Malbet, G. Weigelt et al., Astron. Astrophys. 464, 1 (2007)
Author information
Authors and Affiliations
Corresponding author
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 2009 Springer Science + Business Media B.V.
About this paper
Cite this paper
Ohnaka, K., Driebe, T., Weigelt, G., Wittkowski, M. (2009). Multi-epoch VLTI/MIDI Observations of the Carbon-rich Mira Star V Oph. In: Moorwood, A. (eds) Science with the VLT in the ELT Era. Astrophysics and Space Science Proceedings. Springer, Dordrecht. https://doi.org/10.1007/978-1-4020-9190-2_20
Download citation
DOI: https://doi.org/10.1007/978-1-4020-9190-2_20
Publisher Name: Springer, Dordrecht
Print ISBN: 978-1-4020-9189-6
Online ISBN: 978-1-4020-9190-2
eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)