(1) R.D. Suenram, F.J. Lovas, G.T. Fraser and K. Matsumura, J. Chem. Phys. 92, 4725-4733 (1990).Author Institution: Department of Chemistry, The University of British ColumbiaThe pure rotational spectra of ZrS and ZrO have been recorded using cavity Fourier transform microwave spectroscopy in the frequency range 9-26 GHz. The molecules were generated by laser ablation of a solid Zr rod with 0.05\% of $H_{2}S$ or $O_{2}$, respectively, in either argon or neon. For ZrS, this is the first measurement of the pure rotational spectrum of the $X^{1}\Sigma^{+}$ state. Rotational transitions in the ground vibrational state were observed for all five $Zr^{32}S$ isotopomers and for the $^{90}Zr^{34}S$ isotopomer in natural abundance. Transitions in th...
Author Institution: Department of Chemistry and Biochemistry, Department of Astronomy, and Steward O...
Author Institution: University of Arizona, Department of Chemistry and Biochemitry and Steward Obser...
Zirconium oxide (ZrO) is an important astrophysical molecule that defines the S-star classification ...
Author Institution: National Institute of Standards and Technology, Optical Technology Division; Nat...
Author Institution: Department of Physics and Astronomy, University of British Columbia; Department ...
$^{1}$ J. G. Phillips and S. P. Davis, Astrophys. J. 234, 393 (1979).Author Institution: Department ...
1. B. Simard, S.A. Mitchell, L.M. Hendel, and P.A. Hackett, Faraday Disscuss. Chem. Soc. 86, 163 (19...
The pure rotational spectrum of ZnBr ($^{2}$$\Sigma$$^{+}$) has been recorded using millimeter-wave ...
The pure rotational spectrum of ZnBr (X2Σ+) has been recorded in the frequency range 259-310 GHz usi...
$^{a}$ Present address: Creo Inc., 3755 Willingdon Avenue, Burnaby, BC, Canada V5G 3H3Author Institu...
Pure rotational spectroscopy is one of the highest resolution techniques available for studying gas-...
Several rotational transitions of zinc hydride and deuteride within the £ 0 level of the X 2S / st...
The (0,0) band of the B 2Σ +-X 2Σ + transition of ZrN between 404.1 and 407.1 nm was recorded and ro...
$^{(1)}$ M. Bogey, M. Winnewisser and J.J. Christiansen, to be published.Author Institution: Physika...
Author Institution: Laser Chemistry Group, Division of Chemistry, National Research Council of Canad...
Author Institution: Department of Chemistry and Biochemistry, Department of Astronomy, and Steward O...
Author Institution: University of Arizona, Department of Chemistry and Biochemitry and Steward Obser...
Zirconium oxide (ZrO) is an important astrophysical molecule that defines the S-star classification ...
Author Institution: National Institute of Standards and Technology, Optical Technology Division; Nat...
Author Institution: Department of Physics and Astronomy, University of British Columbia; Department ...
$^{1}$ J. G. Phillips and S. P. Davis, Astrophys. J. 234, 393 (1979).Author Institution: Department ...
1. B. Simard, S.A. Mitchell, L.M. Hendel, and P.A. Hackett, Faraday Disscuss. Chem. Soc. 86, 163 (19...
The pure rotational spectrum of ZnBr ($^{2}$$\Sigma$$^{+}$) has been recorded using millimeter-wave ...
The pure rotational spectrum of ZnBr (X2Σ+) has been recorded in the frequency range 259-310 GHz usi...
$^{a}$ Present address: Creo Inc., 3755 Willingdon Avenue, Burnaby, BC, Canada V5G 3H3Author Institu...
Pure rotational spectroscopy is one of the highest resolution techniques available for studying gas-...
Several rotational transitions of zinc hydride and deuteride within the £ 0 level of the X 2S / st...
The (0,0) band of the B 2Σ +-X 2Σ + transition of ZrN between 404.1 and 407.1 nm was recorded and ro...
$^{(1)}$ M. Bogey, M. Winnewisser and J.J. Christiansen, to be published.Author Institution: Physika...
Author Institution: Laser Chemistry Group, Division of Chemistry, National Research Council of Canad...
Author Institution: Department of Chemistry and Biochemistry, Department of Astronomy, and Steward O...
Author Institution: University of Arizona, Department of Chemistry and Biochemitry and Steward Obser...
Zirconium oxide (ZrO) is an important astrophysical molecule that defines the S-star classification ...