. ▁The ▁inter orb ital ▁sept um ▁was ▁more ▁del icate , ▁with ▁a ▁larger ▁hole ▁in ▁its ▁centre . ▁The ▁bill ▁was ▁about ▁ ▁long , ▁less ▁cur ved ▁and ▁proportion ally ▁a ▁little ▁deeper ▁than ▁in ▁the ▁ho op oe ▁star ling . ▁It ▁also ▁seems ▁to ▁have ▁had ▁larger ▁nost r ils , ▁with ▁the ▁nost ril ▁open ings ▁in ▁the ▁b one ▁being ▁ ▁in ▁length . ▁The ▁mand ible ▁was ▁about ▁ ▁long ▁and ▁ ▁deep ▁proxim ally . ▁The ▁sk ull ▁had ▁an ▁attachment ▁scar ▁above ▁the ▁temporal ▁f ossa . ▁The ▁sup ra oc cip ital ▁r idge ▁on ▁the ▁sk ull ▁was ▁quite ▁strongly ▁developed , ▁and ▁a ▁b iv enter ▁mus cle ▁attachment ▁in ▁the ▁par iet al ▁region ▁below ▁it ▁was ▁consp ic uous . ▁This ▁indicates ▁that ▁the ▁star ling ▁had ▁strong ▁neck ▁and ▁j aw ▁mus cles . ▁ ▁According ▁to ▁Gün ther ▁and ▁Newton , ▁the ▁ul na ▁of ▁the ▁Rod rig ues ▁star ling ▁was ▁somewhat ▁shorter ▁than ▁that ▁of ▁the ▁ho op oe ▁star ling , ▁meas uring ▁; ▁the ▁hum er us ▁measured ▁, ▁and ▁the ▁ke el ▁on ▁its ▁stern um ▁was ▁a ▁bit ▁lower . ▁It ▁had ▁strong ▁qu ill ▁kn obs ▁on ▁the ▁ul na , ▁indicating ▁that ▁the ▁secondary ▁rem iges ▁were ▁well ▁developed . ▁One ▁cor ac oid ▁measured ▁ ▁in ▁length , ▁and ▁one ▁car p omet ac arp us ▁was ▁ ▁long . ▁The ▁leg ▁and ▁feet ▁had ▁the ▁same