Table 2
Summary of available data at mm-cm wavelengths; the new observations presented in this work are highlighted.
| λ | Synthesized beama | Peakb | Flux | rmsc | Ref.d | |
| (mm) | (arcsec, deg) | (mJy) | (mJy) | (mJy) | ||
|
|
||||||
| 0.87 | 0.85 × 0.45, 95 | 253 | 421 | 9 | (1) | |
| 1.3 | ... | ... | 221 | 40 | (2) | |
| 1.3 | 1.5 | ... | 162 | 2 | (3) | |
| 1.3 | 2 | ... | 143 | 8.4 | (4) | |
| 1.3 | 0.45 × 0.29, 35 | 18 | 103 | 1 | (1) | |
| 2.7 | 0.91 × 0.56, 34 | 9 | 22 | 0.3 | (1) | |
| 2.7 | ... | ... | 18 | 0.6 | (2) | |
| 3.4 | ... | ... | 13.1 | 0.5 | (3) | |
| 6.9 | 0.92 × 0.72, –37 | 1.0 | 2.0 | 0.1 | (5) | |
| 13.4 | 0.33 × 0.30, 2 | 0.08 | 0.28 | 0.02 | (1) | |
| 35.7 | 0.91 × 0.81, –15 | 0.046 | 0.079 | 0.009 | (1) | |
| 62.5 | 31 × 23, 49 | <0.75 | ... | 0.25 | (6) | |
Notes.
The first two values correspond to the size of the axes of the synthesized beam ellipse, while the third to its position angle. The beam is reported only for interferometric observations.
In the case of data reduced in this work the rms is extracted directly from the residual noise in final cleaned image, otherwise it is the uncertainty reported in literature.
Data from the literature: (1): this work; (2): Mannings & Sargent (1997); (3): Chapillon et al. (2008); (4): Mannings & Sargent (2000); (5): Testi et al. (2003); (6): Testi et al. (2001).
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