molecules:ism:ti-oxide

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molecules:ism:ti-oxide [2019/10/18 13:17] muellermolecules:ism:ti-oxide [2020/12/10 11:38] (current) – [Titanium Monoxide] mueller
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 by\\ by\\
 L. A. Hillenbrand, G. R. Knapp, D. L. Padgett, L. M. Rebull, and P. M. McGehee,\\ L. A. Hillenbrand, G. R. Knapp, D. L. Padgett, L. M. Rebull, and P. M. McGehee,\\
-//Astron. J.// **143**, Art. No. 37 (2012).+//Astron. J.// **143**, Art. No. 37 (2012).\\
  
 More recently, the\\ More recently, the\\
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 and tentatively toward V899 Aql and RX Psc were reported by\\ and tentatively toward V899 Aql and RX Psc were reported by\\
 K. Smolders, T. Verhoelst, P. Neyskens, J. A. D. L. Blommaert, L. Decin, H. van Winckel, S. van Eck, G. C. Sloan, J. Cami, S. Hony, P. De Cat, J.Menu, and J. Vos.\\ K. Smolders, T. Verhoelst, P. Neyskens, J. A. D. L. Blommaert, L. Decin, H. van Winckel, S. van Eck, G. C. Sloan, J. Cami, S. Hony, P. De Cat, J.Menu, and J. Vos.\\
-A temperature of 600 K was estimated. Even if it is rather uncertain, it is again compatible with circumstellar origin of the emission.+A temperature of 600 K was estimated. Even if it is rather uncertain, it is again compatible with circumstellar origin of the emission.\\
  
-Finally, the detection of rotational transitions in the circumstellar envelope of VY CMa (and others) will be described in the **TiO<sub>2</sub>** section.+Finally, the detection of rotational transitions in the circumstellar envelope of VY CMa (and others) will be described in the **TiO<sub>2</sub>** section.\\
  
 +T. Danilovich, C. A. Gottlieb, L. Decin, A. M. S. Richards, K. L. K. Lee, T. Kamiński, N. A. Patel, K. H. Young, and K. M. Menten\\
 +investigated\\
 +**[[https://doi.org/10.3847/1538-4357/abc079|Rotational Spectra of Vibrationally Excited AlO and TiO in Oxygen-rich Stars]]**\\
 +//Astrophys. J.// **904**, Art. No. 110 (2020).\\
 +//J// = 11 → 10 transitions of TiO with Ω = 1, 2, and 3 were found in the circumstellar envelope of R Doradus up to //v// = 2 and that of IK Tauri up to //v// = 1.\\
  
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-Contributor(s): H. S. P. Müller; 03, 2013; 03, 2017+Contributor(s): H. S. P. Müller; 03, 2013; 03, 2017; 12, 2020
  
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