Observations de pulsateurs compacts à l'aide de la caméra Mont4K CCD

Les pulsateurs compacts sont des étoiles présentant des variations intrinsèques de luminosité dont les gravités de surface sont supérieures à 100,000 cm/s² On retrouve parmi ces objets deux familles des sous-naines chaudes de type B (sdB) pulsantes et quatre familles distinctes de naines blanches pulsantes. Dans le but d'observer les pulsations de tels objets pour ensuite analyser leur propriétés grâce à l'astéroséismologie, l'Université de Montréal, en collaboration avec le Imaging Technology Laboratory (ITL - University of Arizona), a développé la caméra Mont4K (Montreal4K) CCD qui est, depuis le printemps 2007, le principal détecteur employé au télescope Kuiper de 1.55 m du Mt Bigelow (Steward Observatory, University of Arizona). à l'aide de ce montage, des observations ont été menées pour quelques-uns de ces pulsateurs compacts. La première cible fut HS 0702+6043, un pulsateur hybride. Une importante mission pour cet objet, réalisée du 1er novembre 2007 au 14 mars 2008, a permis d'identifier 28 modes de pulsations pour cet objet en plus de mettre en évidence pour certains de ces modes d'importantes variations d'amplitude. Deux autres cibles furent les naines blanches pulsantes au carbone de type « Hot DQ » SDSS J220029.08-074121.5 et SDSS J234843.30-094245.3. Il fut possible de montrer de façon indirecte la présence d'un fort champ magnétique à la surface de J220029.08-074121.5 grâce à la présence de la première harmonique du mode principal. En outre, pour ces deux cibles, on a pu conclure que celles-ci font bel et bien partie de la classe des naines blanches pulsantes au carbone.

Calculs de modèles d'atmosphères hors-ETL avec métaux pour les étoiles de type sdO : le cas particulier de SDSS J1600+0748

Nous présentons nos grilles de modèles d'atmosphères pour les étoiles sous-naines chaudes de type O (sdO) soit : des modèles classiques hors-ETL H, He, des modèles hors-ETL avec, en plus, du C, N, O et finalement des modèles incluant C, N, O, Fe. En utilisant les raies de Balmer et d'hélium dans le domaine du visible, nous avons fait des comparaisons entre les spectres théoriques de nos différentes grilles afin de caractériser les effets des métaux. On trouve que ces effets dépendent à la fois de la température et de la gravité. De plus, l'abondance d'hélium a une influence importante sur les effets des métaux; une abondance d'hélium faible (log N(He)/N(H) < -1,5) occasionne des effets assez importants alors qu'une abondance plus élevée tend à réduire ces mêmes effets. Nous avons aussi trouvé que l'ajout du fer (en abondance solaire) ne cause que des changements relativement faibles à la structure en température et, par le fait même, aux profils des raies d'hydrogène et d'hélium, par rapport aux changements déjà produits par le C, N, O (en abondance solaire). Nous avons utilisé nos grilles pour faire une analyse spectroscopique du spectre à haut signal sur bruit (180) et basse résolution (9 Å) de SDSS J160043.6+074802.9 obtenu au télescope Bok. Notre meilleure ajustement a été obtenu avec notre grille de spectres synthétiques incluant C, N, O et Fe en quantité solaire, menant aux paramètres suivants : Teff = 68 500 ± 1770 K, log g = 6,09 ± 0,07, and log N(He)/N(H) = -0,64 ± 0,05, où les incertitudes proviennent uniquement de la procédure d'ajustement. Ces paramètres atmosphériques, particulièrement la valeur de l'abondance d'hélium, placent notre étoile dans une région où les effets des métaux ne sont pas très marqués.

Modèles d'atmosphères hors-ETL avec métaux : applications aux étoiles sous-naines chaudes

Avec la mise en place dans les dernières années d'une grappe d'ordinateurs (CALYS) dédiés aux calculs de modèles stellaires pour notre groupe de recherche, il nous est désormais possible d'exploiter à leur plein potentiel les modèles d'atmosphères hors équilibre thermodynamique local (HETL) en y incluant des éléments métalliques. Ce type de modèles, plutôt exigeant en temps de calcul, est toutefois essentiel pour analyser correctement les spectres d'étoiles chaudes comme les sous-naines de type O (sdO). Les travaux effectués dans le cadre de cette thèse ont comme point commun l'utilisation de tels modèles d'atmosphères pour faire l'analyse spectroscopique d'étoiles sous-naines chaudes dans des contextes variés. Le coeur de cette thèse porte sur Bd+28 4211, une étoile standard de type sdO très chaude, dans laquelle le problème des raies de Balmer, qui empêche de reproduire ces dernières avec une unique, et réaliste, combinaison de paramètres atmosphériques, est bien présent. Dans un premier temps nous présentons une analyse approfondie de son spectre ultraviolet (UV). Cela nous permet de déterminer les abondances de métaux dans l'atmosphère de l'étoile et de contraindre sa température effective et sa gravité de surface. Par la suite, ces résultats servent de point de départ à l'analyse du spectre optique de l'étoile, dans lequel le problème des raies de Balmer se fait sentir. Cette analyse nous permet de conclure que l'inclusion des abondances métalliques propres à l'étoile dans les modèles d'atmosphères HETL n'est pas suffisant pour surmonter le problème des raies de Balmer. Toutefois, en y incluant des abondances dix fois solaires, nous arrivons à reproduire correctement les raies de Balmer et d'hélium présentes dans les spectres visibles lors d'un ajustement de paramètres. De plus, les paramètres résultants concordent avec ceux indiqués par le spectre UV. Nous concluons que des sources d'opacité encore inconnues ou mal modélisées sont à la source de ce problème endémique aux étoiles chaudes. Par la suite nous faisons une étude spectroscopique de Feige 48, une étoile de type sdB pulsante particulièrement importante. Nous arrivons à reproduire très bien le spectre visible de cette étoile, incluant les nombreuses raies métalliques qui s'y trouvent. Les paramètres fondamentaux obtenus pour Feige 48 corroborent ceux déjà présents dans la littérature, qui ont été obtenus avec des types de modèles d'atmosphères moins sophistiqués, ce qui implique que les effets HETL couplés à la présence de métaux ne sont pas importants dans l'atmosphère de cette étoile particulière. Nous pouvons donc affirmer que les paramètres de cette étoile sont fiables et peuvent servir de base à une future étude astérosismologique quantitative. Finalement, 38 étoiles sous-naines chaudes appartenant à l'amas globulaire omega Centauri ont été analysées afin de déterminer, outre leur température et gravité de surface, leurs abondances d'hélium et de carbone. Nous montrons qu'il existe une corrélation entre les abondances photosphériques de ces deux éléments. Nous trouvons aussi des différences entre les étoiles riches en hélium de l'amas du celles du champ. Dans leur ensemble, nos résultats remettent en question notre compréhension du mécanisme de formation des sous-naines riches en hélium.

Air pollution levels measured at traffic hot spots : Brisbane urban corridor study

Air pollution levels were monitored continuously over a period of 4 weeks at four sampling sites along a busy urban corridor in Brisbane. The selected sites were representative of industrial and residential types of urban environment affected by vehicular traffic emissions. The concentration levels of submicrometer particle number, PM2.5, PM10, CO, and NOx were measured 5-10 meters from the road. Meteorological parameters and traffic flow rates were also monitored. The data were analysed in terms of the relationship between monitored pollutants and existing ambient air quality standards. The results indicate that the concentration levels of all pollutants exceeded the ambient air background levels, in certain cases by up to an order of magnitude. While the 24-hr average concentration levels did not exceed the standard, estimates for the annual averages were close to, or even higher than the annual standard levels.

Thermal analysis and hot stage Raman spectroscopy of the basic copper arsenate mineral : euchroite

The thermal analysis of euchroite shows two mass loss steps in the temperature range 100 to 105°C and 185 to 205°C. These mass loss steps are attributed to dehydration and dehydroxylation of the mineral. Hot stage Raman spectroscopy (HSRS) has been used to study the thermal stability of the mineral euchroite, a mineral involved in a complex set of equilibria between the copper hydroxy arsenates: euchroite Cu2(AsO4)(OH).3H2O → olivenite Cu2(AsO4)(OH) → strashimirite Cu8(AsO4)4(OH)4.5H2O → arhbarite Cu2Mg(AsO4)(OH)3. Hot stage Raman spectroscopy inolves the collection of Raman spectra as a function of the temperature. HSRS shows that the mineral euchroite decomposes between 125 and 175 °C with the loss of water. At 125 °C, Raman bands are observed at 858 cm-1 assigned to the ν1 AsO43- symmetric stretching vibration and 801, 822 and 871 cm-1 assigned to the ν3 AsO43- (A1) antisymmetric stretching vibration. A distinct band shift is observed upon heating to 275 °C. At 275 °C the four Raman bands are resolved at 762, 810, 837 and 862 cm-1. Further heating results in the diminution of the intensity in the Raman spectra and this is attributed to sublimation of the arsenate mineral. Hot stage Raman spectroscopy is most useful technique for studying the thermal stability of minerals especially when only very small amounts of mineral are available.

Thermogravimetric analysis and hot stage Raman spectroscopy of cubic indium hydroxide

The transition of cubic indium hydroxide to cubic indium oxide has been studied by thermogravimetric analysis complimented with hot stage Raman spectroscopy. Thermal analysis shows the transition of In(OH)3 to In2O3 occurs at 219°C. The structure and morphology of In(OH)3 synthesised using a soft chemical route at low temperatures was confirmed by X-ray diffraction and scanning electron microscopy. A topotactical relationship exists between the micro/nano-cubes of In(OH)3 and In2O3. The Raman spectrum of In(OH)3 is characterised by an intense sharp band at 309 cm-1 attributed to ν1 In-O symmetric stretching mode, bands at 1137 and 1155 cm-1 attributed to In-OH δ deformation modes, bands at 3083, 3215, 3123 and 3262 cm-1 assigned to the OH stretching vibrations. Upon thermal treatment of In(OH)3 new Raman bands are observed at 125, 295, 488 and 615 cm-1 attributed to In2O3. Changes in the structure of In(OH)3 with thermal treatment is readily followed by hot stage Raman spectroscopy.

Bonding of aluminum alloy by hot-dipping tin coating

This paper presents bonding technology of aluminum alloy by hot-dipping tin. The dissolution curve of copper in molten tin liquid was obtained in the experiment of hot-dipping Sn. Optimal hot-dipping parameter which was suitable for soldering was designed. To elucidate characteristics of interfacial evolution, the microstructure of the coatings, soldered joint were analyzed using optical microscopy, SEM and EDX. The shear strength of soldered joints was tested as high as 39.9Mpa, which is high enough to achieve the requirement of electronic industry.

New criteria for evaluating methods of identifying hot spots

Identification of hot spots, also known as the sites with promise, black spots, accident-prone locations, or priority investigation locations, is an important and routine activity for improving the overall safety of roadway networks. Extensive literature focuses on methods for hot spot identification (HSID). A subset of this considerable literature is dedicated to conducting performance assessments of various HSID methods. A central issue in comparing HSID methods is the development and selection of quantitative and qualitative performance measures or criteria. The authors contend that currently employed HSID assessment criteria—namely false positives and false negatives—are necessary but not sufficient, and additional criteria are needed to exploit the ordinal nature of site ranking data. With the intent to equip road safety professionals and researchers with more useful tools to compare the performances of various HSID methods and to improve the level of HSID assessments, this paper proposes four quantitative HSID evaluation tests that are, to the authors’ knowledge, new and unique. These tests evaluate different aspects of HSID method performance, including reliability of results, ranking consistency, and false identification consistency and reliability. It is intended that road safety professionals apply these different evaluation tests in addition to existing tests to compare the performances of various HSID methods, and then select the most appropriate HSID method to screen road networks to identify sites that require further analysis. This work demonstrates four new criteria using 3 years of Arizona road section accident data and four commonly applied HSID methods [accident frequency ranking, accident rate ranking, accident reduction potential, and empirical Bayes (EB)]. The EB HSID method reveals itself as the superior method in most of the evaluation tests. In contrast, identifying hot spots using accident rate rankings performs the least well among the tests. The accident frequency and accident reduction potential methods perform similarly, with slight differences explained. The authors believe that the four new evaluation tests offer insight into HSID performance heretofore unavailable to analysts and researchers.

Identifying large truck hot spots using crash counts and PDOEs

Large trucks are involved in a disproportionately small fraction of the total crashes but a disproportionately large fraction of fatal crashes. Large truck crashes often result in significant congestion due to their large physical dimensions and from difficulties in clearing crash scenes. Consequently, preventing large truck crashes is critical to improving highway safety and operations. This study identifies high risk sites (hot spots) for large truck crashes in Arizona and examines potential risk factors related to the design and operation of the high risk sites. High risk sites were identified using both state of the practice methods (accident reduction potential using negative binomial regression with long crash histories) and a newly proposed method using Property Damage Only Equivalents (PDOE). The hot spots identified via the count model generally exhibited low fatalities and major injuries but large minor injuries and PDOs, while the opposite trend was observed using the PDOE methodology. The hot spots based on the count model exhibited large AADTs, whereas those based on the PDOE showed relatively small AADTs but large fractions of trucks and high posted speed limits. Documented site investigations of hot spots revealed numerous potential risk factors, including weaving activities near freeway junctions and ramps, absence of acceleration lanes near on-ramps, small shoulders to accommodate large trucks, narrow lane widths, inadequate signage, and poor lighting conditions within a tunnel.

Transition of chromium oxyhydroxide nanomaterials to chromium oxide : a hot stage Raman spectroscopic study

The transition of disc-like chromium hydroxide nanomaterials to chromium oxide nanomaterials has been studied by hot stage Raman spectroscopy. The structure and morphology of α-CrO(OH) synthesised using hydrothermal treatment was confirmed by X-ray diffraction and transmission electron microscopy. The Raman spectrum of α-CrO(OH) is characterised by two intense bands at 823 and 630 cm-1 attributed to ν1 CrIII-O symmetric stretching mode, bands at 1179 cm-1 attributed to CrIII-OH δ deformation modes. No bands are observed above 3000 cm-1. The absence of characteristic OH vibrational bands may be due to short hydrogen bonds in the α-CrO(OH) structure. Upon thermal treatment of α-CrO(OH), new Raman bands are observed at 599, 542, 513, 396, 344 and 304 cm-1, which are attributed to Cr2O3. This hot-stage Raman study shows that the transition of α-CrO(OH) to Cr2O3 occurs before 350 °C.

Transition of synthetic chromium oxide gel to crystalline chromium oxide : a hot stage Raman spectroscopic study

Chromium oxide gel material was synthesised and appeared to be X-ray amorphous. The changes in the structure of the synthetic chromium oxide gel were investigated using hot-stage Raman spectroscopy based upon the results of thermogravimetric analysis. The thermally decomposed product of the synthetic chromium oxide gel in nitrogen atmosphere was confirmed to be crystalline Cr2O3 as determined by the hot-stage Raman spectra. Two bands were observed at 849 and 735 cm-1 in the Raman spectrum at 25 °C, which were attributed to the symmetric stretching modes of O-CrIII-OH and O-CrIII-O. With temperature increase, the intensity of the band at 849 cm-1 decreased, while the band at 735 cm-1 increased. These changes in intensity are attributed to the loss of OH groups and formation of O-CrIII-O units in the structure. A strongly hydrogen bonded water H-O-H bending band was found at 1704 cm-1 in the Raman spectrum of the chromium oxide gel, however this band shifted to around 1590 cm-1 due to destruction of the hydrogen bonds upon thermal treatment. Six new Raman bands were observed at 578, 540, 513, 390, 342 and 303 cm-1 attributed to the thermal decomposed product Cr2O3. The use of the hot-stage Raman microscope enabled low-temperature phase changes brought about through dehydration and dehydroxylation to be studied.

Environmental health risk assessment of dioxin exposure through foods in a Dioxin hot spot—Bien Hoa City, Vietnam

This study used the Australian Environmental Health Risk Assessment Framework to assess the human health risk of dioxin exposure through foods for local residents in two wards of Bien Hoa City, Vietnam. These wards are known hot-spots for dioxin and a range of stakeholders from central government to local levels were involved in this process. Publications on dioxin characteristics and toxicity were reviewed and dioxin concentrations in local soil, mud, foods, milk and blood samples were used as data for this risk assessment. A food frequency survey of 400 randomly selected households in these wards was conducted to provide data for exposure assessment. Results showed that local residents who had consumed locally cultivated foods, especially fresh water fish and bottom-feeding fish, free-ranging chicken, duck, and beef were at a very high risk, with their daily dioxin intake far exceeding the tolerable daily intake recommended by the WHO. Based on the results of this assessment, a multifaceted risk management program was developed and has been recognized as the first public health program ever to have been implemented in Vietnam to reduce the risks of dioxin exposure at dioxin hot-spots.