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Table 2

Results from Gaussian fit (points B–E with two components) to individual spectra with a spatial resolution of 15.9″ sampled at 7.55″.

Pos. RA Dec v T P FWHM
(J2000) (J2000) [km s-1] [K] [km s-1]

A 5h40′53″ − 2°27′37″ 10.5 21.1 1.4
B 5h41′00″ − 2°20′27″ 12.0 22.5 3.6
14.2 6.9 1.2
C 5h41′00″ − 2°19′34″ 11.3 6.1 1.2
12.2 16.2 4.6
D 5h41′05″ − 2°20′42″ 10.7 9.5 2.7
13.2 16.1 1.9
E 5h41′02″ − 2°26′44″ 10.0 12.4 1.1
12.6 17.4 2.5
F 5h41′06″ − 2°30′46″ 13.0 21.9 2.1
G 5h41′14″ − 2°28′38″ 12.4 20.3 2.3
H 5h41′33″ − 2°30′53″ 11.8 8.1 4.5
I 5h41′24″ − 2°31′16″ 11.3 13.9 2.6

Notes. Positions are indicated in Fig. 1. Listed are the velocity of the peak, the peak temperature, and the full width at half maximum (FWHM) of the peak. Note to spectrum I: from a Lorentzian fit we obtain TP = 15.6 K, which fits the spectrum better by eye; velocity and FWHM are similar.

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