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Home All issues Volume 499 / No 1 (May III 2009) A&A, 499 1 (2009) 163-173 Full HTML
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Table 3:

Measured interstellar polarization parameters of the field stars and estimated foreground polarization toward RY Tauri.
Object Parallax Distance $p_{\rm max}$ $\lambda_{\rm max}$ $\theta _{5500}$ $\theta'$
  [mas] [pc] [%] $[{\rm\AA}]$ [deg] $[ 10^{-3 }\ {\rm deg\ \AA^{-1}}]$
HIP 20728 $7.45 \pm 1.48$ $134.2\pm26.7$ $0.44 \pm 0.02$ $4735 \pm 573$ $167.9 \pm 0.9$ $ -1.2\pm 0.9$
HIP 20250 $9.53 \pm 0.92$ $104.9\pm 10.1$ $0.13 \pm 0.01$ $5082 \pm 789$ $ 3.8 \pm 1.8$ $ -1.7\pm 1.2$
HIP 20262 $4.91 \pm 1.06$ $203.7\pm 44.0$ $1.30 \pm 0.01$ $5250 \pm 173$ $ 4.4 \pm 0.2$ $ -2.2\pm 0.2$
HIP 20324 $4.62 \pm 0.97$ $216.5\pm 45.4$ $2.93 \pm 0.01$ $5752 \pm 35$ $ 14.2 \pm 0.0$ $ 0.1\pm 0.0$
HIP 20663 $4.77 \pm 1.07$ $209.6\pm 47.0$ $0.95 \pm 0.01$ $5301 \pm 1099$ $ 19.8 \pm 0.2$ $-0.2\pm 0.1$
RY Tauri (HIP 20387) Foreground $7.49\pm 2.18$ 139+10-9 a $0.73 \pm 0.36$ $5244 \pm 373$ $ 6.0 \pm 12.0$ $ -1.0\pm 1.0$
a Distance to Taurus-Auriga complex by Bertout et al. (1999).


Source LaTeX | All tables | In the text

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