Rotationally-supported disks around Class I sources in Taurus: disk formation constraints

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Table 6

C¹⁸O J = 2–1 integrated intensities within R_K box as defined in Table 5.

	TMC1A	TMC1	TMR1	L1536

^a [Jy km s^-1]	1.93	0.63	0.26	0.17
M_disk gas	75	24	10	6.8
M_disk dust^b	41–49	4.6–5.4	10–15	19–24

Notes. Disk masses [10^-3M_⊙] inferred from the gas lines and continuum.

^(a)

Typical errors are 0.03–0.04 Jy km s^-1.

^(b)

Disk masses from the range of dust masses obtained with the different methods in Sects. 4.1 and 4.2 with a gas-to-dust ratio of 100.

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