Understanding the multi-wavelength thermal dust polarisation from the Orion molecular cloud in light of the radiative torque paradigm

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Volume 689 (September 2024)

A&A, 689 (2024) A290

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Table 2

Main output parameters of two-phase model.

Regions	f_max × Sin² ψ	β	f_heat	f_scale	χ²
#1	0.53	−4.50	2.14	6.85	0.56
#2	0.29	−3.53	3.06	39.89	10.73
#3	0.57	−4.00	2.13	181.46	3.41
#4	0.58	−4.23	1.53	60.42	2.15
#5	0.69	−4.37	1.24	104.03	2.61
#6	0.94	−4.22	5.37	39.67	5.29
#7	0.94	−4.17	3.42	31.25	3.74
#8	0.58	−4.20	1.70	11.42	2.53
#9	0.16	−3.00	1.84	161.87	2.30
#10	0.32	−3.37	2.50	113.48	16.33
#11	0.34	−3.00	2.35	36.86	18.00
#12	0.38	−3.02	2.31	40.52	26.19

Notes. Similar to Table 1 but for the two-phase model. The total and polarised emission in the second phase are scaled by /Scale and /heat relative to the first phase, with $f_{heat} = T_{dust}^{first - phase} / T_{dust}^{second - phase}$ ${f_{{\rm{heat}}}} = T_{{\rm{dust}}}^{{\rm{first}}-{\rm{phase}}}/T_{{\rm{dust}}}^{{\rm{second}}-{\rm{phase}}}$ .

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