Table 8
Comparison with literature values of Mjet from spatially resolved observations.
Source | log(Ṁjet) | Ref. | Notes |
---|---|---|---|
(M⊙ yr−1) | |||
DG Tau HV | −7.7 | ||
−8.1 | (1) | Total | |
−7.8 | (2) | ||
DG Tau MV | −8.1 | ||
−7.8 | (2) | ||
DO Tau | −8.5 | (HV+MV) | |
−8.3 | (3) | ||
RW Aur A | −7.1 | (HV+MV) | |
−8.7 | (4) | BE | |
CW Tau | −7.9 | ||
−8.4 | (5) | BE | |
HN Tau | −8.2 | ||
−9.3/-8.34 | (6) | (a) | |
RY Tau | −8.3 | ||
−8.6 | (7) | CIV lines | |
−8.8 | (8) | ||
DF Tau HV | −9.2 | ||
HV | -8.85 | (9) | (b) |
DF Tau MV | −9.3 | ||
MV | −8.85 | (9) | (b) |
UY Aur A | −9.5 | ||
−9.3 | (9) | (b) |
Notes. (a)The two values refer to line luminosity and shock method, respectively. (b)Assuming ne = 103 cm−3. Values in boldface are those derived in this work. HV and MV refer to the components at high and medium velocity. BE indicates derivations with the BE technique (Bacciotti & Eislöffel 1999).
References. (1) Maurri et al. (2014), (2) Agra-Amboage et al. (2011), (3) Erkal et al. (2021), (4) Melnikov et al. (2009), (5) Coffey et al. (2008), (6) Hartigan et al. (2004), (7) Skinner et al. (2018), (8) Agra-Amboage et al. (2009), (9) Uvarova et al. (2020).
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