Fig. 3
P% (upper panel) and θ (lower panel) of stars toward L1570 from Bhatt & Jain (1993) (observed without any filter) are compared with those from this work (R-band). The stars are marked with their identification numbers taken from Table 2. Star #97 scattered more from the straight line is found to show (a) Hα emission in its spectra (Sect. 3.3); (b) NIR-excess (Sect. 4.2.1); and (c) intrinsic polarization and polarization angles (Sect. 4.2.1).
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