The coordinated radio and infrared survey for high-mass star formation - III. A catalogue of northern ultra-compact H II regions

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Volume 615 (July 2018)

A&A, 615 (2018) A103

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Table 3

Comparison between velocities (in km s⁻¹) measured inthis work and by Anderson et al. (2009), Table 3 for the sources in common.

CORNISH	v	Anderson	v
G024.4698+00.4954	103	C24.47+0.49	102.67
G024.4721+00.4877	102.8	C24.47+0.49	102.67
G024.4736+00.4950	102.6	C24.47+0.49	102.67
G024.8497+00.0881	109.3	C24.81+0.10	108.31
G030.7661−00.0348	96.1	C30.78−0.03	94.76
G030.7661−00.0348	96.1	U30.84−0.11b	96.89
G031.2420−00.1106	21.1	U31.24−0.11a	21.07
G034.2544+00.1460	57.7	U34.26+0.15	57.1
G034.2571+00.1466	57.7	U34.26+0.15	57.1
G037.9723−00.0965	54.7	C38.05−0.04	54.1
G049.4640−00.3511	59.5	U49.49−0.37	60.08
G049.4891−00.3763	60.9	U49.49−0.37	60.08
G050.3157+00.6747	26.5	U50.32+0.68	26.31

Notes. As the peak channel was used to calculate the velocities, the associated errors are given by the channel width. This equals 0.21 km s⁻¹ for each BU-FCRAO Galactic Ring Survey cube. In practice this error is outweighed by the error due to peculiar motions, which is ~10 km s ⁻¹.

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