Table 15
Stars associated with extended emission.
| HIP | Position angle | Observed diameters | FWHM c | FWHM G | Band | ||
| (arcsec) | (arcsec) | (arcsec) | |||||
|
|
|||||||
| 544 | 102° | 18.0,16.0 | 8.8,7.8 | 8.67 ± 0.10, 8.28 ± 0.10 | 100 μm | ||
| 7978 | 51° | 39.0,28.0 | 15.7,11.3 | 15.5 ± 0.02, 9.02 ± 0.02 | 100 μm | ||
| 13402 | 50° | 19.0,14.0 | 9.2,6.7 | 8.20 ± 0.10, 7.61 ± 0.02 | 100 μm | ||
| 14954(!) | 30° | 18.0,14.0 | 9.4,7.3 | 9.89 ± 0.10, 7.80 ± 0.10 | 100 μm | ||
| 15371 | 98° | 39.0,18.0 | 24.5,11.6 | 20.00 ± 1.0, 12.20 ± 0.36 | 160 μm | ||
| 17439 | 105° | 26.0,14.0 | 13.1,7.1 | 13.35 ± 0.14, 8.68 ± 0.10 | 100 μm | ||
| 22263 | 5° | 21.0,16.0 | 10,7.6 | 10.20 ± 0.10, 8.41 ± 0.09 | 100 μm | ||
| 29271 | 70° | 16.0,10.0 | 14.3,8.9 | 12.00 ± 1.22, 10.00 ± 0.73 | 160 μm | ||
| 32480 | 107° | 34.0,20.0 | 16.0,9.4 | 17.76 ± 0.07, 10.15 ± 0.04 | 100 μm | ||
| 49908 | 50° | 18.0,10.0 | 15.5,8.6 | 13.00 ± 0.94, 11.00 ± 0.60 | 160 μm | ||
| 51502(!) | 0° | 16.0,16.0 | 8.3,8.3 | 9.08 ± 0.12, 8.10 ± 0.11 | 100 μm | ||
| 62207 | 130° | 24.0,14.0 | 13.4,7.8 | 13.13 ± 0.19, 8.40 ± 0.11 | 100 μm | ||
| 72848 | 75° | 21.0,12.0 | 12.7,7.2 | 11.07 ± 0.33, 6.64 ± 0.20 | 100 μm | ||
| 85235 | 0° | 18.0,16.0 | 10.2,9.0 | 10.01 ± 0.23, 9.21 ± 0.21 | 100 μm | ||
| 92043 | 170° | 16.0,10.0 | 19.1,11.9 | 14.00 ± 1.10, 10.00 ± 0.79 | 160 μm | ||
| 107649 | 125° | 17.5,8.0 | 16.1,11.2 | 100 μm | |||
Notes.Column 2 gives the position angles on the sky (from north to east). Column 3 gives the elliptical diameters (major,minor) of the 3σ contours. Column 4 (FWHMc) gives the x and y FWHM values assuming the 3σ contours are Gaussian, while Col. 5 (FWHMG) is a 2D Gaussian fit to the whole detected flux. See text for details. The last column gives the wavelength at which the sizes have been estimated. (!) Stars of the 20–25 pc subsample.
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