Non-ideal magnetohydrodynamics of self-gravitating filaments

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Table 2

Time-averaged mass flux ratio, FWHM ratio, time-averaged mass flux (M_⊙ Myr⁻¹ pc⁻²) and FWHM (pc) at t = 1.0t_ff, for an ideal case, the different inclination angles, magnetic field strengths, and cosmic ray ionization rates.

	Reference	Ideal	θ = 5°	θ = 45°	θ = 90°	no-field	5 μG	20 μG	10⁻¹⁸ s⁻¹	10⁻¹⁶ s⁻¹
	1	0.410	1.372	1.366	0.960	1.684	1.663	0.919	1.317	0.706
FWHM/FWHM_ref	1	7.214	0.575	0.698	1.046	0.534	0.922	1.159	0.755	2.447
	206.15	83.828	282.87	281.55	197.92	347.08	342.802	189.48	271.58	145.58
FWHM	0.023	0.164	0.013	0.016	0.024	0.012	0.022	0.027	0.018	0.057

Notes. Reference case have θ = 77°, B₀ = 10 μG, and ζ = 10⁻¹⁷ s⁻¹. We note that θ = 90° indicates that the magnetic field is perpendicular to the flow, and no-field corresponds to B₀ = 0 μG.

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