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Table 4

Atmosphere parameters and Rb pseudo-dynamical abundances with β = 0.2 and β = 1.2, respectively.

IRAS name Teff (K) log g β (M yr-1) vexp(OH) (km s-1) [Rb/Fe]static [Rb/Fe]dyn [Zr/Fe]dyn

01085+3022 3000* 0.5 0.2 1.0 × 10-7 13 2.0 0.6 0.0
1.2 1.0 × 10-7 0.3

044047427 3000 0.5 0.2 1.0 × 10-7 8 1.3 0.1 0.0
1.2 1.0 × 10-7 0.1

050272158 2800 0.5 0.2 1.0 × 10-7 8 0.4 0.6 +0.5
1.2 1.0 × 10-7 1.1

050986422 3000 0.5 0.2 1.0 × 10-8 6 0.1 0.2 +0.25
1.2 5.0 × 10-7 2.1

05151+6312 3000 0.5 0.2 5.0 × 10-7 15 2.1 0.0 +0.25
1.2 5.0 × 10-7 0.5

06300+6058 3000 0.5 0.2 1.0 × 10-7 12 1.6 0.4 0.0
1.2 1.0 × 10-7 0.3

072222005 3000 0.5 ... ... 8 0.6 ... ...

091944518 3000 0.5 ... ... 11 1.1 ... ...

102615055 3000 0.5 0.2 1.0 × 10-9 4 <1.0 <1.1 +0.25
1.2 1.0 × 10-9 <1.1

142664211 2900 0.5 0.2 5.0 × 10-8 9 0.9 0.1 0.0
1.2 1.0 × 10-7 0.4 0.25

15193+3132 2800 0.5 0.2 1.0 × 10-9 3 0.3 0.4 0.0
1.2 1.0 × 10-9 0.4

155761212 3000 0.5 0.2 1.0 × 10-8 10 1.5 1.0 0.0
1.2 1.0 × 10-8 0.9

160305156 3000 0.5 0.2 1.0 × 10-8 10 1.3 0.6 +0.25
1.2 1.0 × 10-7 0.4

16037+4218 2900 0.5 0.2 1.0 × 10-8 4 0.6 0.5 +0.25
1.2 1.0 × 10-8 0.2

170341024 3300 0.5 0.2 1.0 × 10-8 8 0.2 0.7 0.0
1.2 1.0 × 10-8 0.8

184291721 3000 0.5 0.2 1.0 × 10-8 7 1.2 0.9 +0.25
1.2 5.0 × 10-7 1.0 0.0

190592219 3000 0.5 0.2 1.0 × 10-7 13 2.3 0.5 +0.25
1.2 5.0 × 10-8 0.5

19426+4342 3000 0.5 ... ... 9 1.0 ... ...

20052+0554 3000* 0.5 0.2 5.0 × 10-7 16 1.5 0.0 0.0
1.2 5.0 × 10-7 0.7

200770625 3000 0.5 ... ... 12 1.3 ... ...

203433020 3000 0.5 0.2 1.0 × 10-9 8 0.9 0.7 0.0
1.2 1.0 × 10-9 0.7

Notes. The asterisks indicate that the best fitting Teff in the ZrO 6474 Å spectral region is warmer (3300 K) than the one around the Rb I 7800 Å line (García-Hernández et al. 2006, 2007).

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