Table 1: Candidate target stars for abundance analysis. Rotation velocities from Noterdaeme et al. (in preparation). M? denotes questionable membership, \ensuremath{v\sin i} in ${\rm km~s}^{-1}$. The $\Delta a$ index that is sensitive to CP2 type peculiarity is taken from Maitzen & Catalano (1986). A * indicates stars that were selected for the abundance analysis.
Star sp. type mV \ensuremath{v\sin i} Notes
HD 73722 F5 V 8.92 6.8 *
HD 73778 F0 V 8.76 40 M?
HD 74044 A3 8.48 32 $\Delta a=1$, Am? *
HD 74275 A0 V 7.27 62 *
HD 74535 B8 5.55 37 $\Delta a=26$, Si
HD 75029 A2/3 9.45 24 $\Delta a=-7$, M? *
CPD -52 1568 F5 V 9.62 19  
SHJM 2 F9 10.3 10 PMS? *

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