Missing water in Class I protostellar disks | Astronomy & Astrophysics (A&A)

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Table B.1

DUSTY envelope parameters taken from Kristensen et al. (2012).

Source	p	y ()	τ₁₀₀	r_in	M_env
				(au)	(M_⊙)
Elias 29	1.6	1000	0.1	15.5	0.04
GSS30 IRS1	1.6	1000	0.2	16.2	0.1
TMC1A	1.6	900	0.4	7.7	0.2
L1527	0.9	1200	0.3	5.4	0.9

Notes. τ₁₀₀ is the optical depth at 100 μm that is used to attenuate the stellar spectrum.

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