Properties of dust in the high-latitude translucent cloud L1780 - II. 3D radiative transfer modelling

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Table 1:

Model parameters.
Model	$\lambda_{\rm {fitted}} \left[\mu\rm {m}\right]$	Dust model	Heating	Free parameters^a	$A_{\rm V}^{\rm bg}\left[\rm {mag}\right]$ ^b	$A_{\rm V}^{\rm mod}\left[\rm {mag}\right]$ ^c
A	200	LD	ISRF	N	0.0	4.8
B	100, 200	LD	ISRF	N, $\chi$	0.0	7.1
C	200	LD	ISRF	N	0.5	9.1
D	200	LD	ISRF	N	0.25	6.8
E	100, 200	LD	ISRF	N, $\chi$	0.25	6.7
F	200	LD	ISRF+OB	N	0.25	2.8
G	12, 100, 200	LD+mod.1	ISRF	N, X	0.25	9.1
H	12, 60, 100, 200	LD+mod.2	ISRF	N, X	0.25	8.6

Notes. ^(a) The possible free parameters are the column density N, the scaling of the radiation field, $\chi$ , and the dust abundances, X. ^(b) $A_{\rm V}^{\rm bg}$ refers to additional extinction around the model cloud. ^(c) $A_{\rm V}^{\rm mod}$ is the visual extinction of the model cloud averaged over a 3 $\hbox{$^\prime$ }$ beam.

Source LaTeX | All tables | In the text

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