Early Planet Formation in Embedded Disks (eDisk) - XVI. Asymmetric dust disk driving a multicomponent molecular outflow in the young Class 0 protostar GSS30 IRS3

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Table 3

Results from the SLAM fitting to the position velocity diagram using a single power law.

	¹³CO (2−1)	C¹⁸O (2−1)
Edge method
p_in	0.601 ± 0.010	0.714 ± 0.029
M_b [M_⊙]	0.430 ± 0.004	0.316 ± 0.007
R_b [au]	120.5 ± 1.2	111.0 ± 2.5
	–	8.2

Ridge method
p_in	0.57 ± 0.010	0.655 ± 0.023
M_b [M_⊙]	0.244 ± 0.002	0.211 ± 0.004
R_b ^[au]	${70.45}_{- 0.75}^{+ 0.72}$ $70.45_{ - 0.75}^{ + 0.72}$	73.5 ± 1.5
χ²	25	2.4

Notes. p_in is the power-law index, χ² is the reduced chi-squared of the fit. M_b is the protostellar mass derived given the rotation velocity. R_b is the radius where M_b was measured assuming Keplerian rotation.

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