All Figures

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{odin10_f1.ps} \end{figure}$ Figure 1: Gaussian fits to the weak telluric O₃ ( 30_4, 26-30_3, 27) line during the Odin observations of $\rho ~ {\rm Oph ~ A}$ determined the AOS channel of the line peak (channel width = 0.32 km s^-1). The adopted average channel values for the segments, during which the phase lock was stable, are indicated (see the text).
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{odin10_f2.ps} \end{figure}$ Figure 2: The submm NH₃ (J_K = 1₀-0₀) line (523.66 $\mu$ m) observed with Odin toward $\rho ~ {\rm Oph ~ A}$ (histogram). At 572.5 GHz the Odin $T_{\rm mb}$ -scale is related to the flux density by $F_{\nu }/T_{\rm mb} = 2600$ Jy/K. The quadrupole hyperfine lines in their equilibrium ratios are indicated, together with their total contribution.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{odin10_f1.ps} \end{figure}$	Figure 1: Gaussian fits to the weak telluric O₃ ( 30_4, 26-30_3, 27) line during the Odin observations of $\rho ~ {\rm Oph ~ A}$ determined the AOS channel of the line peak (channel width = 0.32 km s^-1). The adopted average channel values for the segments, during which the phase lock was stable, are indicated (see the text).
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{odin10_f2.ps} \end{figure}$	Figure 2: The submm NH₃ (J_K = 1₀-0₀) line (523.66 $\mu$ m) observed with Odin toward $\rho ~ {\rm Oph ~ A}$ (histogram). At 572.5 GHz the Odin $T_{\rm mb}$ -scale is related to the flux density by $F_{\nu }/T_{\rm mb} = 2600$ Jy/K. The quadrupole hyperfine lines in their equilibrium ratios are indicated, together with their total contribution.
Open with DEXTER