Differences
This shows you the differences between two versions of the page.
Both sides previous revision Previous revision Next revision | Previous revision | ||
molecules:ism:ti-oxide [2019/10/18 13:17] – mueller | molecules:ism:ti-oxide [2020/12/10 11:38] (current) – [Titanium Monoxide] mueller | ||
---|---|---|---|
Line 25: | Line 25: | ||
by\\ | by\\ | ||
L. A. Hillenbrand, | L. A. Hillenbrand, | ||
- | //Astron. J.// **143**, Art. No. 37 (2012). | + | //Astron. J.// **143**, Art. No. 37 (2012).\\ |
More recently, the\\ | More recently, the\\ | ||
Line 32: | Line 32: | ||
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< | + | Finally, the detection of rotational transitions in the circumstellar envelope of VY CMa (and others) will be described in the **TiO< |
+ | 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:// | ||
+ | // | ||
+ | //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.\\ | ||
---- | ---- | ||
Line 57: | Line 62: | ||
---- | ---- | ||
- | Contributor(s): | + | Contributor(s): |
---- | ---- | ||