Top: integrated intensity map of L1495/B213 in N₂H⁺(1−0) adding all hyperfine components. The white contour corresponds to 0.5 K km s^-1. Central position and offsets are as in Fig. 1. First contour and contour interval are 0.5 K km s^-1. Bottom: schematic view of the L1495/B213 complex indicating the regions defined in this paper, which approximately match those of Barnard (1927). The black solid line represents the lowest C¹⁸O(1−0) contour in Fig. 1 and delineates the boundary of the cloud. The red lines represent the N₂H⁺(1−0) emission, which traces the dense cores, and the red labels identify the cores described in Sect. 4 and summarized in Table 2. The stars correspond to stellar objects from the survey of Rebull et al. (2010). Solid symbols represent the youngest objects (Class I and Flat), and open symbols represent evolved objects (Classes II and III).