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Table 4

High ions absorption line shifts and stellar temperatures.

STAR Teff(*) V ion V phot Shift Ref. /Inst.(**)

WD1337+701 20435 –10.5   ±   2.3 –0.3   ±   1.4 –10.2   ±   2.7 1 I
WD0512+326 22750 25   ±  5 20.5   ±  5 4.5   ±   7 2 F
WD0252-055 29120 16.2   ±  5 10.4   ±  5 5.8 V 7 2 F
WD1942+499 33500 6.4   ±  5 7.5   ±  5 –1.1   ±   7 2 F
" " 1  ±   7 7.5   ±   5 –6.5   ±   10 3 C
WD0050-332 34684 13.7   ±  5 18.4   ±  5 –4.7   ±   7 2 F
" " 40.3   ±   1.8 18.4   ±  5 21.9   ±   5 1 I
WD1021+266 35432 13.4   ±  5 12   ±  5 1.4   ±   7 2 F
WD2257-073 38010 50  ±   7 –7.8 (+13.6, –7.5) 57.8   ±   12 3 C
" " 30.8   ±  5 –7.8   ±  5 38.6   ±   7 2 F
WD1611-084 38500 –24.2   ±  5 –35.3   ±  5 11.1   ±   7 2 F
WD2111+498 38866 13.1   ±  5 24.7   ±  5 –11.6   ±   7 2 F
WD1950-432 41339 0.3  ±  5 –26  ±  5 26.3   ±   7 2 F
WD2000-561 44456 –15.3  ±  5 –9.6  ±  5 –5.7   ±   7 2 F
WD0131-164 44850 19.5  ±  5 10.9  ±  5 8.6   ±   7 2 F
WD1029+537 44980 25.7  ±  5 13.8  ±  5 11.9   ±   7 2 F
WD2321-549 45860 –1.6  ±  5 17.5  ±  5 –19.1   ±   7 2 F
WD2011+398 47057 13.9  ±  5 11.1  ±  5 2.8   ±   7 2 F
WD1040+492 47560 35  ±   5 –13.9   ±  5 48.9   ±   7 3 C
" " 45  ±  5 –13.9  ±  5 53.9   ±   7 2 F
WD2124-224 48297 –16.4  ±  5 29.7  ±  5 –46.1   ±   7 2 F
WD0226-615 50000 9.3  ±  5 25.8  ±  5 –16.5   ±   7 2 F
WD2331-475 56682 3  ±  5 28.3  ±  5 –25.3   ±   7 2 F
WD2218+706 56900 –16.3   ±   0.7 –38.7   ±   0.2 22.4   ±   0.7 4 S
WD0501+524 57340 20.4  ±  5 21.5  ±  5 –1.1   ±   7 2 F
WD0455-282 58080 16.2   ±   2.7 69.6   ±   2.0 –53.4  ±   3.5 1 I
" " 59.3  ±  5 57.7  ±  5 1.6   ±   7 2 F
WD0027-636 60595 0.5  ±  5 21.8  ±  5 –21.3   ±   7 2 F
WD0621-376 62280 34.3  ±  5 31.3  ±  5 3   ±   7 2 F
REJ0558-373 63000 7.1   ±   0.8 22.7   ±   2.8 –15.6   ±   3 4 S
WD2211-495 65600 18  ±  5 23.9  ±  5 –5.9   ±   7 2 F
WD1342+442 66750 –12.2  ±  5 –13.1  ±  5 0.9   ±   7 2 F
WD2146-433 67912 10.4  ±  5 27.9  ±  5 –17.5   ±   7 2 F
WD2350-706 69300 10.6  ±  5 40.7  ±  5 –30.1   ±   7 2 F
Ton021 69700 7.6   ±   1.3 37.1   ±   0.2 –29.4   ±   1.3 4 S
WD0501-289 70000 –12.2   ±   4.3 39.3   ±   1.1 –51.5   ±   4.4 1 I
REJ1738+665 71300 –17.8   ±   0.3 30.2   ±   0.3 –48. 0   ±   0.4 4 S
WD1034+001 100000 6.6   ±   2.5 50.8   ±   1.3 –44.4   ±   2.8 1 I
" " 7.9   ±   1.8 51.5   ±   1.9 –43.6   ±     ±   3 G
WD0005+511 120000 –6.2   ±   1.0 36.1   ±   1.7 –42.3   ±   2 1 I
" " –22.5   ±   1.4 F 34.1   ±  2.0 G –56.6   ±   2.4 F/G 3 F/G
WD1159-034 140000 –1.8   ±   3.4 50.1   ±  1.1 –51.8   ±   3.6 1 I
" " und 47.4   ±   1 und 3 F
WD0044-121 150000 –70.2   ±   1.05 –22.0   ±   1.2 –50.2   ±   1.6 1 I
" " –80   ±   1.1 –14   ±   0.8 –66.0   ±   1.4 3 S
WD2117+342 170000 –11.9   ±   1.1 47.2   ±   2.6 –59.1  ±   2.8 1 I
" " –29   ±   2.4 22   ±   4.6 –51   ±   5.2 3 G

Notes. Error bars are taken from the referenced articles or estimated from the present COS measurements. They reflect uncertainties linked to continuum and line fitting and the quality of the signal. They do not include calibration uncertainties, that disappear in the calculation of the velocity shift. (*) References for temperatures are listed in Fig. 5 caption; I = IUE; F = FUSE; C = COS; S = STIS; G = GHRS.

References. (**) 1: Holberg et al. (1998), 2: Barstow et al. (2010), 3: this work, 4: Bannister et al. (2003).

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