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Table 2
Comparison between the W49N and G25.65+1.05 water masers during each flare event.
| Source | Orion | G25.65+ | W49N (3) | W49N (3) | W49N (4) |
|---|---|---|---|---|---|
| KL (1) | 1.05 (2) | ||||
| vpeak | +7.4 | +42.8 | −81 | −81 | +6 |
| (km s−1) | |||||
| Speak | 135 | 120 | 50 | 13 | 80 |
| (kJy) | |||||
| a | −1.55 | −2.19 | −1.01 | −1.65 | −7.98 |
| b | +0.78 | +0.34 | +0.25 | +0.26 | +0.92 |
| Δv0 | 1.1 | 0.7 | 2.0 | 2.0 | 1.0 |
| (km s−1) | |||||
| S0 (Jy) | 20 | 1525 | 154 | 1550 | 15 900 |
| Gain | 8.8 | 4.4 | 5.8 | 2.1 | 1.6 |
| Residual | 0.026 | 0.006 | 0.008 | 0.032 | |
| mean | |||||
| square | |||||
| (σ) |
References. (1) Hirota et al. (2014), (2) Volvach et al. (2019b), (3) Volvach et al. (2019a), (4)this paper.
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