The asteroids whose perihelion distances (q) are smaller than 0.983 AU and aphelion distances (% MathType!MTEF!2!1!+-% feaafeart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn% hiov2DGi1BTfMBaeXafv3ySLgzGmvETj2BSbqefm0B1jxALjhiov2D% aebbfv3ySLgzGueE0jxyaibaiGc9yrFr0xXdbba91rFfpec8Eeeu0x% Xdbba9frFj0-OqFfea0dXdd9vqaq-JfrVkFHe9pgea0dXdar-Jb9hs% 0dXdbPYxe9vr0-vr0-vqpWqaaeaabiGaciaacaqabeaadaqaaqGaaO% qaaiqadgfagaqeaaaa!3D1C!\[\bar Q\]) are larger than 1.017 AU are called Apollo type objects. Similarly Amor type objects are defined by the conditions: 0.987 AU < %="" mathtype!mtef!2!1!+-%="" feaafeart1ev1aaatcvaufebsjuyzl2yd9gzlbvynv2caerbulwbln%="" hiov2dgi1btfmbaexafv3yslgzgmvetj2bsbqefm0b1jxaljhiov2d%="" aebbfv3yslgzguee0jxyaibaigc9yrfr0xxdbba91rffpec8eeeu0x%="" xdbba9frfj0-oqffea0dxdd9vqaq-jfrvkfhe9pgea0dxdar-jb9hs%="" 0dxdbpyxe9vr0-vr0-vqpwqaaeaabigaciaacaqabeaadaqaaqgaao%="" qaaiqadghagaqeaaaa!3d3c!\[\bar="" q\]="">< 1.382="" au="" and="" %="" mathtype!mtef!2!1!+-%="" feaafeart1ev1aaatcvaufebsjuyzl2yd9gzlbvynv2caerbulwbln%="" hiov2dgi1btfmbaexafv3yslgzgmvetj2bsbqefm0b1jxaljhiov2d%="" aebbfv3yslgzguee0jxyaibaigc9yrfr0xxdbba91rffpec8eeeu0x%="" xdbba9frfj0-oqffea0dxdd9vqaq-jfrvkfhe9pgea0dxdar-jb9hs%="" 0dxdbpyxe9vr0-vr0-vqpwqaaeaabigaciaacaqabeaadaqaaqgaao%="" qaaiqadgfagaqeaaaa!3d1c!\[\bar="" q\]=""> 1.666 AU. Both types are peculiar asteroids and have common dynamical behaviors. So, we regard these two type asteroids as one group and try to search for families among them.