Water and ammonia abundances in S140 with the Odin satellite

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Volume 494 / No 2 (February I 2009)

A&A, 494 2 (2009) 637-646

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Table B.2:

13CO Gaussian fits^a. $T_{\rm b}$ uses a source size for the PDR (narrow component) of 120 $^{\prime \prime }$ $\rightarrow \eta _{\rm bf}$ = 2, and a source size for the broad outflow component of 85 $^{\prime \prime }$ $\rightarrow \eta _{\rm bf}$ = 3.
Pos.	$\upsilon_{{\rm LSR}}$	err	$T^{~*}_{{\rm A}}$	$T_{\rm b}$	err	$\Delta \upsilon$	err
	[km s^-1]	[km s^-1]	[mK]	[mK]	[mK]	[km s^-1]	[km s^-1]
1	-7.7	0.04	2665	5920	68	2.8	0.08
2	-7.3	0.02	5877	13 060	56	3.3	0.04
3	-7.3	0.01	6610	14 690	199	3.2	0.07
3	-6.8	0.33	612	2040	207	8.2	1.54
4	-7.3	0.03	3620	8040	66	3.5	0.07
5	-8.2	0.25	1124	2500	282	2.1	0.62

^a Gaussian fits (including errors) to the spectra in 5 positions. For most positions two Gaussians are needed to fit the spectra. Parameters: $\upsilon_{{\rm LSR}}$ = the LSR velocity at the peak temperature, $T^{~*}_{{\rm A}}$ = the amplitude of the Gaussian fit, $\Delta \upsilon$ = FWHM line width.

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