Table 4
Targets properties.
| Name | Hα | FHα | Ratio |
|---|---|---|---|
| (mag) | (10−13 erg s−1 cm−2) | ||
| PDS 70 | 16.71 | 7.5 ± 0.4 | 1.60 |
| J1850-3147 | 16.23 | 9.1 ± 0.8 | 1.42 |
| V1094 Sco | 18.08 | 6.3 ± 0.1 | 2.47 |
| HD 100546 | 11.51 | 4312.5 ± 35.3 | 5.63 |
| HD 163296 | 12.13 | 1799.0 ± 43.0 | 3.28 |
Notes. Columns 2 and 3 give the apparent stellar Hα flux observed by MUSE. We adopt the narrowband filter (N_Ha) used in ZIMPOL to measure the stellar brightness at Hα, listed in Col. 2. We convert the flux unit to AB magnitude system using,
The
FH α is line flux obtained from single Gaussian fitting. Column 4 lists the ratio of peak line flux to continuum flux. All the measurements are observed results without the correction for possible dust extinction from the disk.
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