We present photoelectric photometry of λ And never before published, obtained between February 1982 and December 1990 at 29 different observatories. Then we combine it with all other photometry available to us (previously published, contained in the I.A.U. Commission 27 Archives, and obtained with the Vanderbilt 16-inch automatic telescope but not yet published), to yield a 14.8-year data base. Analysis reveals a long-term cycle in mean brightness, with a full range of 0m.15 and a period of 11.4 ± 0.4 years. Because most of our new photometry was concentrated in the 1983-84 observing season, we analyze that one well-defined light curve with a two-spot model. Spot A keeps a 0m.04 amplitude throughout four rotation cycles whereas the amplitude of spot B diminishes from 0m.09 down almost to 0m.03. The spot rotation periods were 55d.9 ± 0d.6 and 520d.8 ± 1d.0, respectively.

京都大学 / 0048 / 新制・課程博士 / 博士(理学) / 甲第21572号 / 理博第4479号 / 新制||理||1643(附属図書館) / 京都大学大学院理学研究科物理学・宇宙物理学専攻 / (主査)准教授 野上 大作, 教授 長田 哲也, 教授 嶺重 慎 / 学位規則第4条第1項該当 / Doctor of Science / Kyoto University / DGAM

HSLA-65 steel (6.4 mm thick) was friction stir welded at various welding speeds and spindle speeds. Varying weld parameters provided a range of heat inputs. Impact toughness was evaluated as a function of the different weld parameters and corresponding weld heat inputs. Charpy V-Notch (CVN) tests were conducted in parent material and at both the weld nugget centerline and heat-affected zone (HAZ) locations. The upper shelf CVN impact energy of the weld nugget was above that of the base metal for all weld parameters. The upper shelf impact toughness in the HAZ was largely unaffected by changing weld parameters. The nil-ductility transition (NDT) temperature in the weld nugget increased with increasing heat input. The toughness, with respect to the ductile-to-brittle transition, was negatively affected by the increase in heat input. The NDT temperature in the HAZ did not correlate with heat input. The microstructures and microhardness data were examined. Aspects of variation in the impact energy results were identified as the inhomogeneity of the weld microstructure and the placement of the V-notch. Weld nugget microstructures were more inhomogeneous than base metal. Hardness results showed varying values of hardness from the weld crown to the root, transversely across the weld, and longitudinally along the length. Variation due primarily to the inhomogeneity of the weld microstructure is compounded by the location of the V-notch.

Ce travail de thèse présente la caractérisation physique et cinématique des étoiles actives en rayons X et présumées jeunes du voisinage solaire qui sont les contreparties optiques (catalogue Tycho) des sources X du relevé ROSAT All-Sky Survey. <br /><br />Lors de notre programme d'observations spectroscopiques à haute résolution, plus de 800 étoiles tardives furent observées et un total de plus de 1600 spectres a été obtenu. La majorité des paramètres stellaires a été dérivée de ces spectres en utilisant des spectres synthétiques et la méthode de corrélation croisée. Il s'avère que cet échantillon se compose principalement d'étoiles jeunes ayant un âge inférieur au milliard d'années et d'une importante fraction de systèmes multiples spectroscopiques. De nouveaux membres de courants bien connus dont 5 très bons candidats post-T Tauri furent découverts lors de l'analyse de la cinématique avec nos deux méthodes probabilistes. Une nouvelle concentration d'étoiles jeunes (semblable à l'association TW Hydra) a été détectée dont les étoiles ont un âge de 50 - 100 Ma et sont localisées dans l'hémisphère nord. Contrairement aux hypothèses courantes, la contamination par des étoiles évoluées n'est pas négligeable. La modélisation faite de leur contribution dans le modèle de population stellaire en rayons X de Besançon reproduit assez bien les ordres de grandeurs observés. <br /><br />Par la suite, cette étude permettra une meilleure compréhension de l'histoire récente de la formation d'étoiles dans l'environnement proche du Soleil.

No description available.

For the manufacture of higher strength pipelines to be feasible, a better understanding of the effects of welding on toughness is necessary. Bevel submerged arc welds were performed on X80 grade steel. The subsequent Charpy V-notch (CVN) test results indicated that the notch placement in the various heat affected zone regions, and hence the bead geometry, affected the test results. A series of bead-on-plate (BOP) submerged arc welds then were performed on X70 grade steel plate to determine the effects of current, voltage, heat input, polarity, and waveform manipulation (i.e., balance, offset, and frequency) on both single and tandem weld bead geometry. A new bead profile characteristic, the SP ratio, is proposed to describe weld bead geometry, and its relationship with welding parameters is discussed. Sub-size CVN specimens, pulled from many of the BOP weld coupons, were then tested. The greatest subsize CVN fracture energies were achieved when the bead was produced using lower heat input, and when the bead profile possessed a greater SP ratio. / Materials Engineering

Polarization is a powerful tool for understanding stellar atmospheres and circumstellar environments. Mira and semi-regular variable stars have been observed for decades and some are known to be polarimetrically variable, however, the semi-regular variable V Canes Venatici displays an unusually large, unexplained amount of polarization. We present ten years of optical polarization observations obtained with the HPOL instrument, supplemented by published observations spanning a total interval of about forty years for V CVn. We find that V CVn shows large polarization variations ranging from 1 - 6%. We also find that for the past forty years the position angle measured for V CVn has been virtually constant suggesting a long-term, stable, asymmetric structure about the star. We suggest that this asymmetry is caused by the presence of a stellar wind bow shock and tail, consistent with the star's large space velocity.