Volume 535, November 2011
|Number of page(s)||16|
|Section||Galactic structure, stellar clusters and populations|
|Published online||28 October 2011|
The tables below provide the heliocentric RVs measured using various lines of stars that do not exhibit any clear binary signature.
Radial velocities of WR 20b as measured for the various emission lines in the spectrum.
Radial velocities of MSP 18 measured using various absorption lines and the weak C iii λ 5696 emission line.
Radial velocities of MSP 171 measured using various absorption lines.
Radial velocities of MSP 183 measured using various absorption and emission (E) lines.
Radial velocities of MSP 199, Star B and C measured using the He ii λ 5412 line.
© ESO, 2011
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