期刊
ASTRONOMY & ASTROPHYSICS
卷 551, 期 -, 页码 -出版社
EDP SCIENCES S A
DOI: 10.1051/0004-6361/201220290
关键词
astrochemistry; stars: winds, outflows; circumstellar matter; stars: individual: VY Canis Majoris; line: identification
资金
- Bundesministerium fur Bildung und Forschung (BMBF) [FKZ 50OF0901]
- Smithsonian Institution
- Academia Sinica
- INSU/CNRS (France)
- MPG (Germany)
- IGN (Spain)
We report the first detection of pure rotational transitions of TiO and TiO2 at (sub-)millimeter wavelengths towards the red supergiant VY CMa. A rotational temperature, T-rot, of about 250K was derived for TiO2. Although T-rot was not well constrained for TiO, it is likely somewhat higher than that of TiO2. The detection of the Ti oxides confirms that they are formed in the circumstellar envelopes of cool oxygen-rich stars and may be the seeds of inorganic-dust formation, but alternative explanations for our observation of TiO and TiO2 in the cooler regions of the envelope cannot be ruled out at this time. The observations suggest that a significant fraction of the oxides is not converted to dust, but instead remains in the gas phase throughout the outflow.
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