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ALMA observations of TiO 2 around VY CMa

Abstract : Titanium dioxide, TiO2, is a refractory species that could play a crucial role in the dust-condensation sequence around oxygen-rich evolved stars. We present and discuss the detections of 15 emission lines of TiO2 with ALMA in the complex environment of the red supergiant VY CMa. The observations reveal a highly clumpy, anisotropic outflow in which the TiO2 emission likely traces gas exposed to the stellar radiation field. We find evidence for a roughly east-west oriented, accelerating bipolar-like structure, of which the blue component runs into and breaks up around a solid continuum component. We see a distinct tail to the south-west for some transitions, consistent with features seen in the optical and near-infrared. We find that a significant fraction of TiO2 remains in the gas phase outside the dust-formation zone and suggest that this species might play only a minor role in the dust-condensation process around extreme oxygen-rich evolved stars like VY CMa.
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Contributor : Marie-Paule Pomies <>
Submitted on : Friday, January 13, 2017 - 5:13:12 PM
Last modification on : Thursday, May 27, 2021 - 1:54:06 PM

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Elvire de Beck, Wouter Vlemmings, Sébastien Muller, John H. Black, Eamon O'Gorman, et al.. ALMA observations of TiO 2 around VY CMa. Journal of Physics: Conference Series, IOP Publishing, 2016, 728 (2), 022009. ⟨10.1088/1742-6596/728/2/022009⟩. ⟨hal-01435295⟩



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