The rotational spectrum of TiO2

被引:49
作者
Bruenken, S. [1 ,2 ]
Mueller, H. S. P. [3 ,4 ]
Menten, K. M. [4 ]
McCarthy, M. C. [1 ,2 ]
Thaddeus, P. [1 ,2 ]
机构
[1] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[2] Harvard Univ, Sch Engn & Appl Sci, Cambridge, MA 02138 USA
[3] Univ Cologne, Inst Phys, D-50937 Cologne, Germany
[4] Max Planck Inst Radioastron, D-53121 Bonn, Germany
关键词
ISM : molecules; line : identification; molecular data; radio lines : general; stars : AGB and post-AGB;
D O I
10.1086/528934
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The rotational spectrum of titanium dioxide (TiO2) has been detected by laser-ablation molecular beam Fourier transform microwave spectroscopy. Thirteen b-type rotational transitions up to J = 9 and Ka = 4 were measured for the most abundant isotopic species (TiO2)-Ti-48 in the frequency range 7-42 GHz with accuracies of 1-10 kHz, allowing for the precise determination of rotational and centrifugal distortion parameters. In addition, eight and six rotational transitions of the rare isotopic species (TiO2)-Ti-46 and (TiO2)-Ti-50, respectively, have been recorded in the same frequency range. From the derived spectroscopic parameters, rest frequencies of TiO2 can now be calculated to better than 1 km s(-1) in equivalent radial velocity up to fairly high J and K-a at millimeter wavelengths, enabling radioastronomical searches for this stable, highly polar transition metal dioxide in space. Preliminary results of two searches for TiO2 in space are presented.
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页码:1367 / 1371
页数:5
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