National apprenticeship and training standards for the IUE.

Mode of access: Internet.

The story of General Electric's 1960 negotiations with the IUE.

Mode of access: Internet.

IUE leadership training manual, 1962.

Mode of access: Internet.

The IUE INES System: Improved data extraction procedures for IUE

We present the extraction and processing of the IUE Low Dispersion spectra within the framework of the ESA “IUE Newly Extracted Spectra” (INES) System. Weak points of SWET, the optimal extraction implementation to produce the NEWSIPS output products (extracted spectra) are discussed, and the procedures implemented in INES to solve these problems are outlined. The more relevant modifications are: 1) the use of a new noise model, 2) a more accurate representation of the spatial profile of the spectrum and 3) a more reliable determination of the background. The INES extraction also includes a correction for the contamination by solar light in long wavelength spectra. Examples showing the improvements obtained in INES with respect to SWET are described. Finally, the linearity and repeatability characteristics of INES data are evaluated and the validity of the errors provided in the extraction is discussed.

Evaluación de la incontinencia urinaria de esfuerzo en primigravidas a termino. Seguimiento a los 6, 12 y 24 meses postparto

pag. var.: il.

The Exotic Eclipsing Nucleus of the Ring Planetary Nebula SuWt 2

SuWt 2 is a planetary nebula (PN) consisting of a bright ionized thin ring seen nearly edge-on, with much fainter bipolar lobes extending perpendicularly to the ring. It has a bright (12th magnitude) central star, too cool to ionize the PN, which we discovered in the early 1990s to be an eclipsing binary. Although it was anticipated that there would also be an optically faint, hot, ionizing star in the system, a spectrum from the International Ultraviolet Explorer (IUE) did not reveal a UV source. We present extensive ground-based photometry and spectroscopy of the central binary collected over the ensuing two decades, resulting in the determination that the orbital period of the eclipsing pair is 4.9 days, and that it consists of two nearly identical A1 V stars, each of mass ~2.7 M sun. The physical parameters of the A stars, combined with evolutionary tracks, show that both are in the short-lived "blue-hook" evolutionary phase that occurs between the main sequence and the Hertzsprung gap, and that the age of the system is about 520 Myr. One puzzle is that the stars' rotational velocities are different from each other, and considerably slower than synchronous with the orbital period. It is possible that the center-of-mass velocity of the eclipsing pair is varying with time, suggesting that there is an unseen third orbiting body in the system. We propose a scenario in which the system began as a hierarchical triple, consisting of a ~2.9 M sun star orbiting the close pair of A stars. Upon reaching the asymptotic giant branch stage, the primary engulfed the pair into a common envelope, leading to a rapid contraction of the orbit and catastrophic ejection of the envelope into the orbital plane. In this picture, the exposed core of the initial primary is now a white dwarf of ~0.7 M sun, orbiting the eclipsing pair, which has already cooled below the detectability possible by IUE at our derived distance of 2.3 kpc and a reddening of E(B - V) = 0.40. The SuWt 2 system may be destined to perish as a Type Ia supernova.

Distance limits to intermediate- and high-velocity clouds

We present optical spectra of 403 stars and quasi-stellar objects in order to obtain distance limits towards intermediate- and high-velocity clouds (IHVCs), including new Fibre-fed Extended Range Optical Spectrograph (FEROS) observations plus archival ELODIE, FEROS, High Resolution Echelle Spectrometer (HIRES) and Ultraviolet and Visual Echelle Spectrograph (UVES) data. The non-detection of Ca II K interstellar (IS) absorption at a velocity of −130 to −60 km s−1 towards HDE 248894 (d ∼ 3 kpc) and HDE 256725 (d ∼ 8 kpc) in data at signal-to-noise ratio (S/N) > 450 provides a new firm lower distance limit of 8 kpc for the anti-centre shell HVC. Similarly, the non-detection of Ca II K IS absorption towards HD 86248 at S/N ∼ 500 places a lower distance limit of 7.6 kpc for Complex EP, unsurprising since this feature is probably related to the Magellanic System. The lack of detection of Na I D at S/N = 35 towards Mrk 595 puts an improved upper limit for the Na I column density of log (NNaD <) 10.95 cm−2 towards this part of the Cohen Stream where Ca II was detected by Wakker et al. Absorption at ∼ −40 km s−1 is detected in Na I D towards the Galactic star PG 0039+049 at S/N = 75, placing a firm upper distance limit of 1 kpc for the intermediate-velocity cloud south (IVS), where a tentative detection had previously been obtained by Centurion et al. Ca ´ II K and Na I D absorption is detected at −53 km s−1 towards HD 93521, which confirms the upper distance limit of 2.4 kpc for part of the IV arch complex obtained using the International Ultraviolet Explorer (IUE) data by Danly. Towards HD 216411 in Complex H a non-detection in Na D towards gas with log(NH I) = 20.69 cm−2 puts a lower distance limit of 6.6 kpc towards this HVC complex. Additionally, Na I D absorption is detected at −43.7 km s−1 in the star HD 218915 at a distance of 5.0 kpc in gas in the same region of the sky as Complex H. Finally, the Na I/Ca II and Ca II/H I ratios of the current sample are found to lie in the range observed for previous studies of IHVCs.

The impact of accretion disc winds on the optical spectra of cataclysmic variables

Many high-state non-magnetic cataclysmic variables (CVs) exhibit blueshifted absorption or P-Cygni profiles associated with ultraviolet (UV) resonance lines. These features imply the existence of powerful accretion disc winds in CVs. Here, we use our Monte Carlo ionization and radiative transfer code to investigate whether disc wind models that produce realistic UV line profiles are also likely to generate observationally significant recombination line and continuum emission in the optical waveband. We also test whether outflows may be responsible for the single-peaked emission line profiles often seen in high-state CVs and for the weakness of the Balmer absorption edge (relative to simple models of optically thick accretion discs). We find that a standard disc wind model that is successful in reproducing the UV spectra of CVs also leaves a noticeable imprint on the optical spectrum, particularly for systems viewed at high inclination. The strongest optical wind-formed recombination lines are H alpha and He ii lambda 4686. We demonstrate that a higher density outflow model produces all the expected H and He lines and produces a recombination continuum that can fill in the Balmer jump at high inclinations. This model displays reasonable verisimilitude with the optical spectrum of RW Trianguli. No single-peaked emission is seen, although we observe a narrowing of the double-peaked emission lines from the base of the wind. Finally, we show that even denser models can produce a single-peaked H alpha line. On the basis of our results, we suggest that winds can modify, and perhaps even dominate, the line and continuum emission from CVs.

Protocolo de Treino dos Músculos do Pavimento Pélvico em Mulheres com Incontinência Urinária de Esforço: Revisão Sistemática

Introdução: Os exercícios de fortalecimento dos músculos do pavimento pélvico (EFMPP) são considerados a primeira intervenção no tratamento da incontinência urinária de esforço (IUE), porém os EFMPP são distintos, não existindo evidência sobre os parâmetros de treino. Objetivo: Identificar o protocolo e/ ou os parâmetros de treino dos músculos do pavimento pélvico (MPP) mais eficaz no tratamento da IUE feminina. Método: A pesquisa bibliográfica foi realizada entre janeiro de 1992 a março de 2014 nas bases de dados PubMed, Cochrane Library, PEDro, web of Science e LILACS. Os artigos incluídos eram de língua inglesa, estudos experimentais, no qual comparavam EFMPP com o tratamento placebo, usual ou sem tratamento, com idade compreendida entre os 18 e os 65 anos e diagnóstico de IUE. Os critérios de exclusão abrangeram o diagnóstico de IUE desencadeada por fatores externos ao trato urinário inferior, grávidas, puérperas, prolapso ≥ 2 e outros tipos de IU. A avaliação da qualidade metodológica for realizada através da escala PEDro. Resultados: Sete artigos de elevada qualidade metodológica foram incluídos na presente revisão. A amostra foi constituída por 331 mulheres, com idade média de 44,4 anos, duração média das perdas urinárias de 64 meses e a gravidade da IUE variou entre ligeira a severa. Os programas de EFMPP eram distintos em relação aos parâmetros de treino dos MPP, sendo que alguns estudos incluíram o treino abdominal, supervisão e técnicas adjuvantes. A taxa de curada da quantidade de perda urinária variou entre 28,6 a 80%, enquanto a força dos MPP variou de 15,6% a 161,7%. Conclusão: Na presente revisão sistemática, os EFMPP combinados com palpação digital, biofeedback e cones vaginais parecem ser mais eficazes na redução da quantidade de perda urinária, comparado com os EFMPP isolados ou sem tratamento. Esta revisão permitiu igualmente identificar as 12 semanas de duração da intervenção, 10 repetições por série e diferentes posições, sendo os parâmetros de treino mais consistentes na redução dos sintomas.

Suivi à long terme de l’efficacité d’un traitement de physiothérapie sur l'incontinence urinaire d'effort persistante en période postnatale

L’incontinence urinaire d’effort (IUE) est une condition fréquente en période postnatale pouvant affecter jusqu’à 77% des femmes. Neuf femmes sur dix souffrant d’IUE trois mois après l’accouchement, vont présenter une IUE cinq ans plus tard. Le traitement en physiothérapie de l’IUE par le biais d’un programme d’exercices de renforcement des muscles du plancher pelvien est reconnu comme étant un traitement de première ligne efficace. Les études ont prouvé l’efficacité de cette approche sur l’IUE persistante à court terme, mais les résultats de deux ECR à long terme n’ont pas démontré un maintien de l’effet de traitement. L’effet d’un programme en physiothérapie de renforcement du plancher pelvien intensif et étroitement supervisé sur l’IUE postnatale persistante avait été évalué lors d’un essai clinique randomisé il y a sept ans. Le but principal de la présente étude était d’évaluer l’effet de ce programme sept ans après la fin des interventions de l’ECR initial. Un objectif secondaire était de comparer l’effet de traitement à long terme entre un groupe ayant fait seulement des exercices de renforcement du plancher pelvien et un groupe ayant fait des exercices de renforcement du plancher pelvien et des abdominaux profonds. Un troisième objectif était d’explorer l’influence de quatre facteurs de risques sur les symptômes d’IUE et la qualité de vie à long terme. Les cinquante-sept femmes ayant complétées l’ECR initial ont été invitées à participer à l’évaluation du suivi sept ans. Vingt et une femmes ont participé à l’évaluation clinique et ont répondu à quatre questionnaires, tandis que dix femmes ont répondu aux questionnaires seulement. L’évaluation clinique incluait un pad test et la dynamométrie du plancher pelvien. La mesure d’effet primaire était un pad test modifié de 20 minutes. Les mesures d’effets secondaires étaient la dynamométrie du plancher pelvien, les symptômes d’IUE mesuré par le questionnaire Urogenital Distress Inventory, la qualité de vie mesurée par le questionnaire Incontinence Impact Questionnaire et la perception de la sévérité de l’IUE mesuré par l’Échelle Visuelle Analogue. De plus, un questionnaire portant sur quatre facteurs de risques soit, la présence de grossesses subséquentes, la v présence de constipation chronique, l’indice de masse corporel et la fréquence des exercices de renforcement du plancher pelvien de l’IUE, venait compléter l’évaluation. Quarante-huit pour-cent (10/21) des participantes étaient continentes selon de pad test. La moyenne d’amélioration entre le résultat pré-traitement et le suivi sept ans était de 26,9 g. (écart-type = 68,0 g.). Il n’y avait pas de différence significative des paramètres musculaires du plancher pelvien entre le pré-traitement, le post-traitement et le suivi sept ans. Les scores du IIQ et du VAS étaient significativement plus bas à sept ans qu’en prétraitement (IIQ : 23,4 vs 15,6, p = 0,007) et (VAS : 6,7 vs 5,1, p = 0,001). Les scores du UDI étaient plus élevés au suivi sept ans (15,6) qu’en pré-traitement (11,3, p = 0,041) et en post-traitement (5,7, p = 0,00). La poursuite des exercices de renforcement du plancher pelvien à domicile était associée à une diminution de 5,7 g. (p = 0,051) des fuites d’urine observées au pad test selon une analyse de régression linéaire. Les limites de cette étude sont ; la taille réduite de l’échantillon et un biais relié au désir de traitement pour les femmes toujours incontinentes. Cependant, les résultats semblent démontrer que l’effet du traitement à long terme d’un programme de renforcement des muscles du plancher pelvien qui est intensif et étroitement supervisé, est maintenu chez environ une femme sur deux. Bien que les symptômes d’IUE tel que mesuré par les pad test et le questionnaire UDI, semblent réapparaître avec le temps, la qualité de vie, telle que mesurée par des questionnaires, est toujours meilleure après sept qu’à l’évaluation initiale. Puisque la poursuite des exercices de renforcement du plancher pelvien est associée à une diminution de la quantité de fuite d’urine au pad test, les participantes devraient être encouragées à poursuivre leurs exercices après la fin d’un programme supervisé. Pour des raisons de logistique la collecte de donnée de ce projet de recherche s’est continuée après la rédaction de ce mémoire. Les résultats finaux sont disponibles auprès de Chantale Dumoulin pht, PhD., professeure agrée à l’Université de Montréal.

Étude comparative de la morphologie du plancher pelvien des femmes âgées continentes et avec incontinence urinaire

But: Cette étude a pour but de comparer : a)la morphologie du plancher pelvien (PP), du col vésical et du sphincter urogénital strié (SUS) par IRM et b) la fonction du PP par palpation digitale (PERFECT scheme) chez les femmes âgées continentes ou avec incontinence urinaire à l’effort (IUE) et mixte (IUM). Méthode: Les femmes ont appris à contracter correctement leur PP et la fonction de leur PP a été évaluée. Une séance d’IRM dynamique 3T a suivi. Résultats: 66 femmes ont participé à l’étude. Les groupes étaient similaires en âge, IMC, nombre d’accouchements vaginaux et d’hystérectomie. La validité et la fidélité des différentes mesures anatomiques utilisées ont été confirmées au début de cette étude. Afin de contrôler l’effet potentiel de la taille du bassin sur les autres paramètres, les femmes ont été appariées par la longueur de leur inlet pelvien. Les femmes avec IUM ont un PP plus bas et un support des organes pelviens plus faible, selon leurs ligne M, angle LPC/Ligne H et hauteur de la jonction urétro-vésicale (UV). Les femmes avec IUE ont un PP similaire à celui des continentes, mais présentent plus d’ouverture du col vésical et un angle UV postérieur plus large au repos que les autres groupes. Il n’y a aucune différence de morphologie du SUS entre les groupes. De plus, selon les résultats du PERFECT scheme, les femmes avec IU ont une force du PP plus faible que les continentes. Les femmes avec IUM montrent aussi une faible élévation des muscles du PP à la contraction. Les femmes avec IUE ont, quant à elle, un problème de coordination à la toux. Conclusion: Les déficits causant l’IUE et l’IUM sont différents, mais supportent tous le rationnel des exercices du PP pour le traitement de l’IUE et l’IUM. Ces résultats supportent le besoin de traitements de rééducation spécifiques aux déficits de chacun des types d’IU.

Modelling of Ultraviolet and Vissible Emissions in Comets

Comets are the spectacular objects in the night sky since the dawn of mankind. Due to their giant apparitions and enigmatic behavior, followed by coincidental calamities, they were termed as notorious and called as `bad omens'. With a systematic study of these objects modern scienti c community understood that these objects are part of our solar system. Comets are believed to be remnant bodies of at the end of evolution of solar system and possess the material of solar nebula. Hence, these are considered as most pristine objects which can provide the information about the conditions of solar nebula. These are small bodies of our solar system, with a typical size of about a kilometer to a few tens of kilometers orbiting the Sun in highly elliptical orbits. The solid body of a comet is nucleus which is a conglomerated mixture of water ice, dust and some other gases. When the cometary nucleus advances towards the Sun in its orbit the ices sublimates and produces the gaseous envelope around the nucleus which is called coma. The gravity of cometary nucleus is very small and hence can not in uence the motion of gases in the cometary coma. Though the cometary nucleus is a few kilometers in size they can produce a transient, extensive, and expanding atmosphere with size several orders of magnitude larger in space. By ejecting gas and dust into space comets became the most active members of the solar system. The solar radiation and the solar wind in uences the motion of dust and ions and produces dust and ion tails, respectively. Comets have been observed in di erent spectral regions from rocket, ground and space borne optical instruments. The observed emission intensities are used to quantify the chemical abundances of di erent species in the comets. The study of various physical and chemical processes that govern these emissions is essential before estimating chemical abundances in the coma. Cameron band emission of CO molecule has been used to derive CO2 abundance in the comets based on the assumption that photodissociation of CO2 mainly produces these emissions. Similarly, the atomic oxygen visible emissions have been used to probe H2O in the cometary coma. The observed green ([OI] 5577 A) to red-doublet emission ([OI] 6300 and 6364 A) ratio has been used to con rm H2O as the parent species of these emissions. In this thesis a model is developed to understand the photochemistry of these emissions and applied to several comets. The model calculated emission intensities are compared with the observations done by space borne instruments like International Ultraviolet Explorer (IUE) and Hubble Space Telescope (HST) and also by various ground based telescopes.

Avaliação da incontinência urinária de esforço em mulheres na pós-menopausa com e sem queixa de perda urinária através da aplicação do pad-test de 1 hora

Stress urinary incontinence (SUI) is defined as "involuntary loss of urine" due to several processes that alter the ability of the bladder to hold urine properly, regarded as a social and hygienic problem that adversely affects quality of life. In postmenopausal women, IU is associated with atrophy and weakness of the pelvic floor muscles. The objective this study was investigate, using the onehour pad test, stress urinary leakage (SUI), evaluate and compare their results in postmenopausal and premenopausal women. The survey was characterized as a cross-sectional study. The study consisted of 60 postmenopausal women were divided into GIU - consisting of 34 volunteers complaining of involuntary loss of urine during stress - and GSIU - consisting of 26 volunteers without complaints of loss of urine during stress, and 15 women, during the premenopausal (GPM), and ovulatory with normal menstrual cycle. All volunteers were evaluated clinically, subjected to one-hour pad test, after the biochemical evaluation of blood and sex hormones. Statistical analysis was performed by descriptive analysis, ANOVA, Turkey´s post-test and Pearson correlation. The results showed that 100% of postmenopausal patients had involuntary loss of urine during one hour pad test (GIU: 4.0 g; GSIU: 4.5 g). GPM remained continent after an hour pad test (GPM: 0.4 g). In addition, Pearson showed a strong correlation between urine loss with time since menopause (r = 0.8, p <0.01) and body mass index - BMI (r = 0.7; p = 0.01). These data suggest that the one-hour pad test is a useful test to assess and quantify urinary leakage, including those volunteers who had no previous complaint of SUI

Urodinâmica convencional versus cistometria simplificada para caracterização da incontinência urinária feminina

OBJETIVO: avaliar a concordância dos diferentes parâmetros urodinâmicos comparados à cistometria simplificada, permitindo uma diminuição na relação custo-benefício no diagnóstico da incontinência urinária de esforço (IUE) na mulher. MÉTODOS: foram coletadas e avaliadas retrospectivamente as informações contidas dos prontuários de trinta pacientes acompanhadas, no período de janeiro de 2000 a março de 2001. Todas foram submetidas a exame físico geral e ginecológico. O estudo urodinâmico foi realizado pela técnica convencional, utilizando-se aparelho Dynograph Recorder R-611. A cistometria simplificada foi realizada com auxílio de um equipo em Y de PVC (pressão venosa central), conectado a um sonda de Foley 14 F, que permitia tanto a infusão de soro fisiológico como a captação da pressão intra-vesical. Foram analisados os parâmetros: volume residual, capacidade vesical, complacência, presença de contrações involuntárias do detrusor e perdas urinárias aos esforços. Para determinação da proporção de concordância entre os métodos foram utilizados o teste de concordância de Pearson e o teste de Wilcoxon, para amostras relacionadas. RESULTADOS: a média de idade foi de 50 anos, com extremos variando de 28 a 70 anos. O índice de concordância entre os estudos, na demonstração das perdas urinárias aos esforços, foi de 67%. Para a detecção das contrações involuntárias do detrusor, a proporção de concordância foi de 90%. A média do volume residual encontrado na cistometria simplificada foi de 16,8 ml contra 2 ml da urodinâmica convencional, com diferença significativa (p < 0,01). A média de capacidade vesical máxima no estudo urodinâmico foi de 440,5 ml, enquanto que, na cistometria simplificada, foi de 387 ml (p < 0,05). A complacência vesical foi, em média, significativamente maior na cistometria simplificada (43,0 ml/cmH2O) quando comparada ao estudo urodinâmico (31,5 ml/cmH2O), com p < 0,01. CONCLUSÃO: Avaliações preliminares sugerem que a propedêutica uroginecológica associada à cistometria simplificada é uma opção a ser considerada na avaliação clínica e pré-operatória de pacientes com IUE em substituição à urodinâmica convencional, particularmente onde esta última não se encontra disponível. A cistometria simplificada é um exame acessível que é capaz de detectar contrações involuntárias do detrusor, assim como identificar perdas urinárias com relativa sensibilidade, proporcionando ao examinador noções fidedignas do comportamento vesical.

Comparison of active and passive forces of the pelvic floor muscles in women with and without stress urinary incontinence

Background: The reduction of the pelvic floor muscles (PFM) strength is a major cause of stress urinary incontinence (SUI). Objective: To compare active and passive forces, and vaginal cavity aperture in continent and stress urinary incontinent women. Method: The study included a total of thirty-two women, sixteen continent women (group 1 - G1) and sixteen women with SUI (group 2 - G2). To evaluate PFM passive and active forces in anteroposterior (sagittal plane) and left-right directions (frontal plane) a stainless steel specular dynamometer was used. Results: The anteroposterior active strength for the continent women (mean +/- standard deviation) (0.3 +/- 0.2 N) was greater compared to the values found in the evaluation of incontinent women (0.1 +/- 0.1 N). The left-right active strength (G1=0.43 +/- 0.1 N; G2=0.40 +/- 0.1 N), the passive force (G1=1.1 +/- 0.2 N; G2=1.1 +/- 0.3 N) and the vaginal cavity aperture (G1=21 +/- 3 mm; G2=24 +/- 4 mm) did not differ between groups 1 and 2. Conclusion: The function evaluation of PFM showed that women with SUI had a lower anteroposterior active strength compared to continent women.