Model exploration of near-IR ro-vibrational CO emission as a tracer of inner cavities in protoplanetary disks

Home

All issues

Volume 637 (May 2020)

A&A, 637 (2020) A29

Full HTML

Free Access

Table 1

Disk model series.

Series	Varied parameter	TTauri values	Herbig values	Other changing parameters
(1)	R_in [au]	0.05, 0.1, 0.5, 1.0, 5.0, 10.0, 15.0	0.1, 0.365, 0.5, 1.0, 5.0, 10.0,	–
			15.0, 20.0, 25.0, 30.0
(2)	ɛ	−1.5, −1.0, −0.5, 0.0, 0.5,	−1.5, −1.0, −0.5,	–
		0.75, 1.0, 1.25, 1.75	−0.25, 0.0, 1.0, 1.5
(3)	M_gas [M_⊙]	0.00001, 0.001, 0.01, 0.05, 0.1	0.00001, 0.001, 0.01, 0.05, 0.1	d/g
(4)	d/g	0.001, 0.01, 0.1, 1.0, 10.0, 100.0	0.001, 0.01, 0.1, 1.0, 10.0, 100.0	M_disk
(5)	R_in+M_gas [au, M_⊙]		1.0 & 0.001 (a), 5.0 & 0.001 (b)	d/g
(6)	d∕g+δ_C		0.1 & 7.08 (c), 0.1 & 6.08 (d),	–
			1.0 & 7.08 (e), 1.0 & 6.08 (f)

Notes. Bold font numbers are values for the standard model. The only model series that uses the large CO molecule is series 1.

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.