Linear polarization of submillimetre masers - Tracing magnetic fields with ALMA

Free Access

Table 3

Fixed parameter values assumed in our numerical models.

Molecule	g	Γ	gΩ_1G^a	B^b	ΔΩ
		(s^-1)	(s^-1)	(G)	(sr)


SiO	0.155	5	1480.96	1	10^-2
H₂O	0.65	1	6226.22	0.05	10^-2
HCN	0.098	1	957.8	1	10^-2

Notes.

^(a)

Values calculated using Eq. (2) for a magnetic field B = 1 G.

^(b)

Magnetic field of the same order of magnitude as the values detected towards SFRs and CSE of late-type stars for regions at densities of n_H₂ = 10¹⁰ cm^-3 in the case of SiO and HCN, and n_H₂ = 10⁸ cm^-3 in the case of H₂O.

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.