Rats with removal of the motor cortex in adulthood were compared behaviorally and neuroanatomically with rats with similar removals at 4 days of age. The results suggest that neonatal ablation of the motor cortex of rats is more debilitating behaviorally than similar injury in adulthood and produces abnormal morphogenesis of the posterior neocortex. Neonatal lesions of the motor cortex produced more chronic abnormalities in movements of the distal effectors that accompany adult lesions (tongue, snout, and digit use) and, in addition, produced abnormalities in limb placement on a narrow beam and a significant impairment in spatial learning, neither of which is associated with adult lesions. When the brains of neonatally operated rats were compared with those of control rats or rats operated on in adulthood, there were striking differences. Although the area of cavity appeared smaller in the neonatal operates, their brains weighed less, the neocortex was thinner, and the cross-sectional area of the remaining cortex was reduced, when compared with those of the adult-operated group. It is suggested that studies of the acquisition of various neuropsychological learning tasks may have greatly overestimated the degree of sparing following anterior neocortical lesions in rats.

We present an overview of current needs for accurate laboratory atomic transition probabilities (log(gf)) for astrophysical applications, particularly for iron group element spectra in the IR, optical, UV, and VUV spectral regions. Examples are given of our recent measurements, undertaken using the combination of high-resolution Fourier transform spectrometry and time-resolved laser-induced fluorescence. Laboratory measured log(gf) values are particularly important for the determination of elemental abundances in astrophysical objects. Advances in astronomical instrumentation, particularly access to underexplored regions (IR, vacuum UV,VUV), require improved accuracy and completeness of the atomic database for meaningful analyses of astrophysical spectra.

We report a new study of the V I atom using a combination of time-resolved laser-induced fluorescence and Fourier transform spectroscopy that contains newly measured radiative lifetimes for 25 levels between 24,648 cm −1 and 37,518 cm −1 and oscillator strengths for 208 lines between 3040 and 20000 Å from 39 upper energy levels. Thirteen of these oscillator strengths have not been reported previously. This work was conducted independently of the recent studies of neutral vanadium lifetimes and oscillator strengths carried out by Den Hartog et al. and Lawler et al., and thus serves as a means to verify those measurements. Where our data overlap with their data, we generally find extremely good agreement in both level lifetimes and oscillator strengths. However, we also find evidence that Lawler et al. have systematically underestimated oscillator strengths for lines in the region of 9000 ± 100 Å. We suggest a correction of 0.18 ± 0.03 dex for these values to bring them into agreement with our results and those of Whaling et al. We also report new measurements of hyperfine structure splitting factors for three odd levels of V I lying between 24,700 and 28,400 cm −1 .

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