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Table 5

Radial velocities of the cool and hot X-ray emitting plasmas in the Chandra (vXc and vXh) and in the Stellar ( and ) reference frames.

Star v E a v phot b v Xc v Xh
(Heliocentric Ref. frame) (Chandra ref. frame) (Stellar Ref. frame)

Method 1: individual line positions

TW Hya (1) 11.8 12.4 38.9 ± 5.1 19.9 ± 6.9 38.3 ± 5.1 19.3 ± 6.9
TW Hya (2) –21.3 12.4 73.1 ± 16.4 38.8 ± 23.2 39.3 ± 16.4 5.1 ± 23.2
AU Mic –28.2 –4.1 21.5 ± 6.5 17.4 ± 7.1 − 2.6 ± 6.5 − 6.7 ± 7.1
EV Lac (1) 2.7 0.5 − 9.9 ± 5.3 5.9 ± 5.3 − 7.8 ± 5.3 8.1 ± 5.3
EV Lac (2) –4.8 0.5 8.2 ± 6.6 16.9 ± 6.9 2.8 ± 6.6 11.5 ± 6.9
AD Leo –28.5 12.4 46.6 ± 7.2 40.1 ± 7.6 5.7 ± 7.2 − 0.8 ± 7.6
β Cet 27.2 13.3 − 31.5 ± 5.4 − 19.1 ± 2.2 − 17.6 ± 5.4 − 5.2 ± 2.2
λ And –20.2 7.0 18.9 ± 4.7 24.8 ± 3.2 − 8.3 ± 4.7 − 2.4 ± 3.2
ξ Uma 23.7 –18.2 − 52.7 ± 4.6 − 48.9 ± 3.4 − 10.8 ± 4.6 − 7.0 ± 3.4
24 Uma –17.6 –27.0 − 3.9 ± 9.9 − 11.4 ± 4.7 5.5 ± 9.9 − 2.0 ± 4.7

Method 2: spectral model parameter estimation

TW Hya (1) 11.8 12.4 44.0 ± 2.0 25.0 ± 6.0 43.4 ± 2.0 24.4 ± 6.0

Notes. All the velocities are in km s-1. All the errors refer to the 1σ level.

(a)

Radial velocity of the Earth, computed at the time corresponding to the middle between the start and the stop of each observation.

(b)

Radial photospheric velocity of each star.

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