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Home All issues Volume 494 / No 2 (February I 2009) A&A, 494 2 (2009) 637-646 Full HTML
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Table B.1:

Observed transitions and their parametersa in S140 with the Odin satellite in a five point NE-SW strip.
Species Transition Freq $E_{\rm u}$ A-coeff $\Delta \upsilon$ Pos. $\upsilon_{{\rm LSR}}$ $T_{\rm peak}$ $\int$ $T^{~*}_{{\rm A}}$ d$\upsilon$ rms note
    [GHz] [K] [s-1] [kms-1]   [kms-1] [mK] [K kms-1] [mK]  
H2O 11,0-10,1 556.936 61.0 3.46e-3 0.27 1 -8.0 207 0.64 39  
            2 -6.9 517 2.74 68  
            3 -6.6 632 3.34 19  
            4 -7.0 379 1.84 57  
            5 - - - 44 No detection.
H218O 11,0-10,1 547.676 60.5 3.29e-3 0.34 3 - - - $\sim$8 No detection.
CO 5-4 576.258 83.0 1.22e-5 0.32 1 -5.4 6680 47.1 67  
            2 -5.0 11 760 94.2 47  
            3 -5.5 13 240 108.8 43  
            4 -6.6 8690 60.1 50  
            5 -6.9 2220 10.1 160  
13CO 5-4 550.926 79.3 1.10e-5 0.27 1 -7.8 2 740 8.29 115  
            2 -7.4 5930 21.4 81  
            3 -7.4 7110 27.7 61  
            4 -7.6 3640 13.2 119  
            5 -8.5 1190 2.5 291  
NH3 10-00 572.498 27.5 1.61e-3 0.32 1 -8.0 444 1.18 99  
            2 -7.4 467 1.83 33  
            3 -7.4 588 2.66 29  
            4 -7.3 381 1.86 36  
            5 - - - 91 No detection
a Transition = the quantum numbers for the transition; Freq = rest frequency of the transition; $E_{\rm u}$ = the upper state energy; A-coeff = the Einstein A-coefficient; $\Delta \upsilon$ = the velocity resolution; Pos = the strip position from NE to SW. $\upsilon_{{\rm LSR}}$ = the peak LSR velocity; $T_{\rm peak}$ = the observed peak temperature of the transition; $\int$  $T^{~*}_{{\rm A}}$ d$\upsilon$ = the integrated intensity from the observed spectra not corrected for beam-efficiency or beam-filling; rms = noise.

Source LaTeX | All tables | In the text

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