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

D. Harsono; J. K. Jørgensen; E. F. van Dishoeck; M. R. Hogerheijde; S. Bruderer; M. V. Persson; J. C. Mottram

doi:10.1051/0004-6361/201322646

Home

All issues

Volume 562 (February 2014)

A&A, 562 (2014) A77

Full HTML

Free Access

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.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.