The halo of M 105 and its group environment as traced by planetary nebula populations - II. Using kinematics of single stars to unveil the presence of intragroup light around the Leo I galaxies NGC 3384 and M 105

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Fig. 2.

Comparison of the velocity measurements obtained for PNe that lie in the areas of intersection of the two fields. The grey shaded regions indicate the nominal 1σ and 2σ PN.S velocity uncertainties of ±20 and ±40 km s⁻¹, respectively. For the M 105-W field, ‘prev.’ indicates the previous measurements by H+2020.

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