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.
Type de document :
Article dans une revue
Journal of Physics: Conference Series, IOP Publishing, 2016, 728 (2), pp.id. 022009. <10.1088/1742-6596/728/2/022009>
Liste complète des métadonnées

https://hal.archives-ouvertes.fr/hal-01435295
Contributeur : Marie-Paule Pomies <>
Soumis le : vendredi 13 janvier 2017 - 17:13:12
Dernière modification le : mercredi 2 août 2017 - 10:11:17

Identifiants

Collections

Citation

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), pp.id. 022009. <10.1088/1742-6596/728/2/022009>. <hal-01435295>

Partager

Métriques

Consultations de la notice

229