We have derived abundances for 54 elements in the extreme roAp star HD 101065. ESO spectra with a resolution of about 80 000, and S/N of 200 or more were employed. The adopted model has Teff=6600 K, and log(g)=4.2. Because of the increased line opacity and consequent low gas pressure, convection plays no significant role in the temperature structure. Lighter elemental abundances through the iron group scatter about standard abundance distribution (SAD) (solar) values. Iron and nickel are about one order of magnitude deficient while cobalt is enhanced by 1.5 dex. Heavier elements, including the lanthanides, generally follow the solar pattern but enhanced by 3 to 4 dex. Odd‐Z elements are generally less abundant than their even‐Z neighbours. With a few exceptions (e.g. Yb), the abundance pattern among the heavy elements is remarkably coherent, and resembles a displaced solar distribution.

Stent patients had significantly lower acute complications compared with surgery patients or BA patients, although they were more likely to require a planned reintervention. At short-term and intermediate follow-up, stent and surgical patients achieved superior hemodynamic and integrated aortic arch imaging outcomes compared with BA patients. Because of the nonrandomized nature of this study, these results should be interpreted with caution.

Context. Despite the importance of magnetic fields to a full understanding of the properties of accreting Herbig Ae/Be stars, these fields have scarcely been studied until now over the rotation cycle. One reason for the paucity of these observations is the lack of knowledge of their rotation periods. The sharp-lined young Herbig Ae star HD 101412 with a strong surface magnetic field has become in the past few years one of the most well-studied targets among the Herbig Ae/Be stars. Aims. We present our multi-epoch polarimetric spectra of this star acquired with FORS 2 to search for a rotation period and constrain the geometry of the magnetic field. Methods. We measured longitudinal magnetic fields for 13 different epochs distributed over 62 days. These new measurements and our previous measurements of the magnetic field in this star were combined with available photometric observations to determine the rotation period. Results. We find the rotation period to be P = 42.076 ± 0.017 d. According to near-infrared imaging studies, the star is observed nearly edge-on. The star exhibits a single-wave variation in the longitudinal magnetic field during the stellar rotation cycle. These observations are usually considered as evidence of a dominant dipolar contribution to the magnetic field topology.

Background-The purpose of this study was to compare the long-term outcomes of children randomized to surgery or balloon angioplasty (BA) for native coarctation (CoA). A prior randomized, short-term comparison of BA and surgery for native CoA in 36 children demonstrated equivalent relief of obstruction. The risk of aneurysm formation and possibly restenosis was higher among patients treated with BA. Methods and Results-Blood pressure, residual aortic obstruction, and exercise performance were evaluated. Need for repeat intervention was reviewed. Aortic arch anatomy was assessed with magnetic resonance angiography. For subjects who were not available to return for evaluation, the most recent clinical record was utilized. Among the 36 subjects initially randomized, 21 returned for evaluation (11 BA, 10 surgery). The average time since initial intervention to evaluation for all subjects was 10.6Ϯ4.7 years for BA subjects and 11.3Ϯ3.7 years for surgical subjects. Resting blood pressure, CoA gradient, exercise performance, MRI analysis of the aortic arch, and need for repeat interventions were not different for the 2 treatment strategies. There was a higher incidence of aneurysm formation (35% versus 0%) and a greater difference in blood pressure between the right and left legs with exercise among BA subjects. Some aneurysms developed late, first being detected more than 5 years after the initial intervention. Only 50% of BA subjects remained free of both aneurysm formation and repeat intervention compared with 87.5% of surgical subjects (Pϭ0.03). Conclusions-BA for the treatment of childhood CoA is associated with a higher incidence of aneurysm formation and iliofemoral artery injury than surgery. These differences should be considered when undertaking treatment for native CoA during childhood.

The objective of this study was to evaluate the potential role of B-type natriuretic peptide (BNP) levels in children with congenital heart disease undergoing cardiac catheterization. Measurement of plasma BNP concentration has been shown to be useful in the diagnosis, risk stratification, and management of adult patients with congestive heart failure, but little is known about the role of BNP in children with structural congenital heart disease. We measured plasma BNP levels using the Triage BNP test in patients with congenital heart disease referred for diagnostic or interventional cardiac catheterization. Plasma BNP concentration was measured in 96 children and 11 adults > or = 19 years old (7.9+/-8.3 years) undergoing heart catheterization for underlying congenital heart disease. BNP levels ranged from < 5 to > 1300 pg/ml, with a median BNP concentration of 19.0 pg/ml. Baseline BNP concentrations were > 100.0 pg/ml on 19 occasions in 17 patients. The pressure difference between the left ventricle and ascending aorta was 10-110 mmHg in 21 patients. BNP concentrations for this cohort ranged from < 5.0 to 1060.0 pg/ml and correlated with the degree of left ventricular outflow obstruction (correlation coefficient, 0.661; p = 0.001). This study suggests that with additional research, BNP concentration may prove to be a useful clinical tool in managing children and adults with congenital heart disease.

Abstract. The profiles of Hα in a number of cool Ap stars are anomalous. Broad wings, indicative of temperatures in the range 7000-8000 K end abruptly in narrow cores. The widths of these cores are compatible with those of dwarfs with temperatures of 6000 K or lower. This profile has been known for Przybylski's star, but it is seen in other cool Ap stars. The Hβ profile in several of these stars shows a similar core-wing anomaly (CWA). In Przybylski's star, the CWA is probably present at higher Balmer members. We are unable to account for these profiles within the context of LTE and normal dwarf atmospheres. We conclude that the atmospheres of these stars are not "normal". This is contrary to a notion that has long been held.

We present the results of a high spectral resolution study of the eclipsing binary AR Aur. AR Aur is the only known eclipsing binary with a HgMn primary star exactly on the zero‐age main sequence (ZAMS) and a secondary star still contracting towards the ZAMS. We detect, for the first time in the spectra of the primary star, that for many elements the line profiles are variable over the rotation period. The strongest profile variations are found for the elements Pt, Hg, Sr, Y, Zr, He and Nd, while the line profiles of O, Na, Mg, Si, Ca, Ti and Fe show only weak distortions over the rotation period. The slight variability of He and Y is also confirmed by the study of high‐resolution spectra of another HgMn star: α And. A preliminary modelling of the inhomogeneous distribution has been carried out for Sr and Y. Our analysis shows that these elements are very likely concentrated in a fractured ring along the rotational equator. It may be an essential clue for the explanation of the origin of the chemical anomalies in HgMn stars (which are very frequently found in binary and multiple systems) that one large fraction of the ring is missing exactly on the surface area which is permanently facing the secondary, and another small one on the almost opposite side. The results presented about the inhomogeneous distribution of various chemical elements over the stellar surface of the primary suggest new directions for investigations to solve the question of the origin of abundance anomalies in B‐type stars with HgMn peculiarity.

Low weight does not affect survival or reintervention rates after coarctation repair in neonates and infants less than 3 months of age. Balloon angioplasty is an effective treatment for recurrent obstruction after coarctation repair in infancy. In the current era, timing of the operation should be based on clinical status.