Grain alignment and dust evolution physics with polarisation (GRADE-POL) - I. Dust polarisation modelling for isolated starless cores

Open Access

Fig. 5

Left panel: relation between $A_{V}^{l o s s}$ $A^{\rm loss}_{\rm V}$ , where the grain completely loses its alignment, and maximum grain size. This plot is shown for several commonly used wavelengths from optical to near-IR. Right panel: relationship between the wavelength of peak starlight polarisation, λ_max, and A_V. The value of λ_max increases initially and then remains steady as A_V increases.

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