Star | Stellar parametersa determined by | Stellar model parameters adopted in this paper | |||
Lecureur et al. (2007) | Zoccali (2009), private comm. |
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|
see also Zoccali et al. (2008) | FWHM in km s-1 | ||||
B3-b1 | 4300/1.7/-0.78/1.5 | 4400/1.7/-0.60/1.3 | 4365/2.0/-0.73/1.5 | +0.3 | 5.0 |
B3-b7 | 4400/1.9/+0.20/1.3 | 4350/1.6/+0.21/1.2 | 4310/2.1/+0.06/1.6 | +0.08 | 4.8 |
B3-b8 | 4400/1.8/-0.62/1.4 | 4350/1.7/-0.65/1.4 | 4250/1.5/-0.69/1.4 | +0.3 | 4.8 |
BW-b6 | 4200/1.7/-0.25/1.3 | 4450/1.9/-0.20/1.4 | 4340/2.2/-0.16/1.5 | +0.15 | 4.3 |
BW-f6 | 4100/1.7/-0.21/1.5 | 4400/1.8/-0.23/1.6 | 4150/1.5/-0.31/1.6 | +0.2 | 5.0 |
B6-f1 | 4200/1.6/-0.01/1.5 | 4250/1.9/-0.08/1.5 | 4030/1.3/-0.08/1.5 | +0.1 | 5.3 |
B6-b8 | 4100/1.6/+0.03/1.3 | 4250/1.8/-0.06/1.4 | 3985/1.1/-0.14/1.3 | +0.1 | 5.7 |
B6-f7 | 4300/1.7/-0.42/1.6 | 4450/1.8/-0.27/1.5 | 4315/1.9/-0.34/1.6 | +0.2 | 4.8 |
Stellar parametersa determined by | Stellar model parameters adopted in this paper | ||||
Fulbright et al. (2007) and used by Ryde et al. (2009) |
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FWHM in km s-1 | |||||
Arp 4203 | 3902/0.5/-1.25/1.9 | 3815/0.35/-1.25/1.8 | +0.35 | 6.2 | |
Arp 4329 | 4197/1.3/-0.90/1.5 | 4153/1.15/-1.02/1.5 | +0.35 | 5.8 | |
Arp 1322 | 4106/0.9/-0.23/1.6 | 4250/1.5/-0.16/1.5 | +0.15 | 6.2 | |
Arcturus | 4290/1.5/-0.5/1.7 | 4280/1.7/-0.53/1.7 | +0.3 | 3.7 |
a The
stellar parameters are given as the effective temperature, ,
in K, the logarithmic surface gravity,
,
in cgs units, and the microturbulence,
,
in km s-1.
b The
macroturbulence is given as the FWHM used in the
final convolution of the synthetic spectra fitted to include both
effects of stellar macroturbulence and the instrumental profile.
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