PKS 1830-211: A Face-On Spiral Galaxy Lens

We present new Hubble Space Telescope images of the gravitational lens PKS 1830-211, which allow us to characterize the lens galaxy and update the determination of the Hubble constant from this system. The I-band image shows that the lens galaxy is a face-on spiral galaxy with clearly delineated spiral arms. The southwestern image of the background quasar passes through one of the spiral arms, explaining the previous detections of large quantities of molecular gas and dust in front of this image. The lens galaxy photometry is consistent with the Tully-Fisher relation, suggesting the lens galaxy is a typical spiral galaxy for its redshift. The lens galaxy position, which was the main source of uncertainty in previous attempts to determine H_0, is now known precisely. Given the current time delay measurement and assuming the lens galaxy has an isothermal mass distribution, we compute H_0 = 44 +/- 9 km/s/Mpc for an Omega_m = 0.3 flat cosmological model. We describe some possible systematic errors and how to reduce them. We also discuss the possibility raised by Courbin et al. (2002), that what we have identified as a single lens galaxy is actually a foreground star and two separate galaxies.Comment: 21 pp., 4 figs., accepted by ApJ, section added to discuss related work by Courbin et al. (astro-ph/0202026

The Quintuple Quasar: Radio and Optical Observations

We present results from high-resolution radio and optical observations of PMN J0134-0931, a gravitational lens with a unique radio morphology and an extremely red optical counterpart. Our data support the theory of Keeton & Winn (2003): five of the six observed radio components are multiple images of a single quasar, produced by a pair of lens galaxies. Multi-frequency VLBA maps show that the sixth and faintest component has a different radio spectrum than the others, confirming that it represents a second component of the background source rather than a sixth image. The lens models predict that there should be additional faint images of this second source component, and we find evidence for one of the predicted images. The previously-observed large angular sizes of two of the five bright components are not intrinsic (which would have excluded the possibility that they are lensed images), but are instead due to scatter broadening. Both the extended radio emission observed at low frequencies, and the intrinsic image shapes observed at high frequencies, can be explained by the lens models. The pair of lens galaxies is marginally detected in HST images. The differential extinction of the quasar images suggests that the extreme red color of the quasar is at least partly due to dust in the lens galaxies.Comment: ApJ, in press. 22 pp, 10 fig

Remissão de sintomas iniciais do declínio de citros pela aplicação de reguladores vegetais

For the experiment 13 year old pera sweet orange on rangpur lime stionic combinations from a plot in the Mogi-Guaçu county, São Paulo State, were choosen. All plants showed in January 1984, unilateral Brazilian decline (blight) symptoms. The diseased state of the plants was further confirmed by low water uptake. The statistically design was by completely randomized blocks, with 6 treatments, 4 replications and 1 tree per plot. The following growth regulator treatments were applied: 1) Check; 2) gibberellic acid (GA) at 100ppm + 2,4-dichlorophenoxyacetic acid (2,4-D) at l0ppm; 3) GA at 50ppm + 2,4-D at 10ppm; 4) GA at 50ppm + NAA at 15ppm + biofertilizer at 1ml/lwater; 6) ethyl-5-chlorine 1 H-3-indazolyl acetate (ethilclozate) at 0,1ml/l water. The products were applied in January 85. The growth regulators were applied as foliar sprays to thoroughly wet the leaves. Five evaluation on the plant reactions were undertaken, respectively at 100,193,276,346 and 405 days from the first application of the products. The results obtained based on a visual score and Kruskal-Wallis test showed that treatments with GA at 50ppm + NAA at 20ppm, GA at 100ppm + 2,4-D at 10ppm, and GA at 50ppm+NAA at 15ppm+ bifertilizer at 1ml/lwater, presented satisfactory degree of symptoms remission that differed statistically from the check. This amelioration however found no parallelism to the results obtained by the water uptake test that still showed low levels. Those figures however were a little higher in the treated plants than in the checks. These experiments will be continued for a few more years to determine whether or not the symptoms remission in the foliage is permanent and will lead eventually to the improvement of the whole plant.Para a instalação do presente experimento foi escolhido um talhão do cultivar de laranja Pera/ limão 'Cravo', de 13 anos, no município de Mogi-Guaçu, Estado de São Paulo. Todas as plantas mostravam em janeiro de 1984, sintomas de declínio inicial unilateral. A ocorrência do declínio foi confirmada pela baixa absorção de água. O delineamento estatístico utilizado foi em blocos ao acaso, com 6 tratamentos e 4 repetições, considerando-se uma planta por parcela. Os seguintes tratamentos com reguladores vegetais foram aplicados em janeiro de 1985: Controle, ácido giberélico (GA) 100ppm + ácido 2,4-diclorofenoxiacético (2,4-D) 10ppm; GA 50ppm + ácido naftalenacético (NAA) 20ppm; GA 50ppm + NAA 15ppm + biofertilizante foliar (Fort Flora-2) 1ml/lde água e etilclozato (Figaron) 0,1ml/lde água. Os reguladores vegetais foram aplicados em pulverização foliar, com cobertura completa das folhas. Cinco avaliações visuais foram realizadas aos 100, 193, 276, 346 e 405 dias da aplicação dos produtos químicos. Os resultados obtidos, baseados na observação visual e no teste de Kruskal-Wallis mostraram que os tratamentos com GA 50ppm + NAA 20ppm; Ga 100ppm + 2,4-D 10ppm e GA 50ppm + NAA 15ppm + biofertilizante foliar 1ml/lde água apresentaram um nível de remissão de sintomas que diferiu estatisticamente do controle. Essa melhoria, todavia, não encontrou paralelismo com os resultados obtidos pelo teste de absorção de água, que mostrou baixos níveis. Entretanto, os níveis de absorção de água das plantas tratadas ainda foram um pouco maiores que nas controle. Esse experimento deverá ser conduzido por mais alguns anos para determinar se a remissão dos sintomas nas folhas é ou não permanente e se poderá levar eventualmente a melhoria de toda a planta

Effectively Mapping Linguistic Abstractions for Message-passing Concurrency to Threads on the Java Virtual Machine

Efficient mapping of message passing concurrency (MPC) abstractions to Java Virtual Machine (JVM) threads is critical for performance, scalability, and CPU utilization; but tedious and time consuming to perform manually. In general, this mapping cannot be found in polynomial time, but we show that by exploiting the local characteristics of MPC abstractions and their communication patterns this mapping can be determined effectively. We describe our MPC abstraction to thread mapping technique, its realization in two frameworks (Panini and Akka), and its rigorous evaluation using several benchmarks from representative MPC frameworks. We also compare our technique against four default mapping techniques: thread-all, round-robin-task-all, random-task-all and work-stealing. Our evaluation shows that our mapping technique can improve the performance by 30%-60% over default mapping techniques. These improvements are due to a number of challenges addressed by our technique namely: i) balancing the computations across JVM threads, ii) reducing the communication overheads, iii) utilizing information about cache locality, and iv) mapping MPC abstractions to threads in a way that reduces the contention between JVM threads

Fully relativistic calculation of magnetic properties of Fe, Co and Ni adclusters on Ag(100)

We present first principles calculations of the magnetic moments and magnetic anisotropy energies of small Fe, Co and Ni clusters on top of a Ag(100) surface as well as the exchange-coupling energy between two single adatoms of Fe or Co on Ag(100). The calculations are performed fully relativistically using the embedding technique within the Korringa-Kohn-Rostoker method. The magnetic anisotropy and the exchange-coupling energies are calculated by means of the force theorem. In the case of adatoms and dimers of iron and cobalt we obtain enhanced spin moments and, especially, unusually large orbital moments, while for nickel our calculations predict a complete absence of magnetism. For larger clusters, the magnitudes of the local moments of the atoms in the center of the cluster are very close to those calculated for the corresponding monolayers. Similar to the orbital moments, the contributions of the individual atoms to the magnetic anisotropy energy strongly depend on the position, hence, on the local environment of a particular atom within a given cluster. We find strong ferromagnetic coupling between two neighboring Fe or Co atoms and a rapid, oscillatory decay of the exchange-coupling energy with increasing distance between these two adatoms.Comment: 8 pages, ReVTeX + 4 figures (Encapsulated Postscript), submitted to PR

23 GHz VLBI Observations of SN 2008ax

We report on phase-referenced 23 GHz Very-Long-Baseline-Interferometry (VLBI) observations of the type IIb supernova SN 2008ax, made with the Very Long Baseline Array (VLBA) on 2 April 2008 (33 days after explosion). These observations resulted in a marginal detection of the supernova. The total flux density recovered from our VLBI image is 0.8$\pm$0.3 mJy (one standard deviation). As it appears, the structure may be interpreted as either a core-jet or a double source. However, the supernova structure could be somewhat confused with a possible close by noise peak. In such a case, the recovered flux density would decrease to 0.48$\pm$0.12 mJy, compatible with the flux densities measured with the VLA at epochs close in time to our VLBI observations. The lowest average expansion velocities derived from our observations are $(1.90 \pm 0.30) \times 10^5$ km s$^{-1}$ (case of a double source) and $(5.2 \pm 1.3) \times 10^4$ km s$^{-1}$ (taking the weaker source component as a spurious, close by, noise peak, which is the more likely interpretation). These velocities are 7.3 and 2 times higher, respectively, than the maximum ejecta velocity inferred from optical-line observations.Comment: 4 pages, 3 figures. Accepted in A&A on 24/03/200

Broad Balmer Wings in BA Hyper/Supergiants Distorted by Diffuse Interstellar Bands: Five Examples in the 30 Doradus Region from the VLT-FLAMES Tarantula Survey

Extremely broad emission wings at Hβ and Hα have been found in VLT-FLAMES Tarantula Survey data for five very luminous BA supergiants in or near 30 Doradus in the Large Magellanic Cloud. The profiles of both lines are extremely asymmetrical, which we have found to be caused by very broad diffuse interstellar bands (DIBs) in the longward wing of Hβ and the shortward wing of Hα. These DIBs are well known to interstellar but not to many stellar specialists, so that the asymmetries may be mistaken for intrinsic features. The broad emission wings are generally ascribed to electron scattering, although we note difficulties for that interpretation in some objects. Such profiles are known in some Galactic hyper/supergiants and are also seen in both active and quiescent Luminous Blue Variables (LBVs). No prior or current LBV activity is known in these 30 Dor stars, although a generic relationship to LBVs is not excluded; subject to further observational and theoretical investigation, it is possible that these very luminous supergiants are approaching the LBV stage for the first time. Their locations in the HRD and presumed evolutionary tracks are consistent with that possibility. The available evidence for spectroscopic variations of these objects is reviewed, while recent photometric monitoring does not reveal variability. A search for circumstellar nebulae has been conducted, with an indeterminate result for one of them

Microgrooves and microrugosities in titanium implant surfaces: an in vitro and in vivo evaluation

This article belongs to the Special Issue Clinical Implants and the Biocompatibility of Biodegradable BiomaterialsThe physical characteristics of an implant surface can determine and/or facilitate osseointegration processes. In this sense, a new implant surface with microgrooves associated with plus double acid treatment to generate roughness was evaluated and compared in vitro and in vivo with a non-treated (smooth) and double acid surface treatment. Thirty disks and thirty-six conical implants manufactured from commercially pure titanium (grade IV) were prepared for this study. Three groups were determined, as described below: Group 1 (G1), where the samples were only machined; group 2 (G2), where the samples were machined and had their surface treated to generate roughness; and test group 3 (G3), where the samples were machined with microgrooves and the surface was treated to generate the roughness. For the in vitro analysis, the samples were submitted to scanning microscopy (SEM), surface profilometry, the atomic force microscope (MFA) and the surface energy test. For the in vivo analyses, thirty-six implants were placed in the tibia of 9 New Zealand rabbits in a randomized manner, after histological and histomorphometric analysis, to determine the level of contact between the bone and implant (BIC%) and the bone area fraction occupancy (BAFO%) inside of the threads. The data collected were statistically analyzed between groups (p < 0.05). The in vitro evaluations showed different roughness patterns between the groups, and the G3 group had the highest values. In vivo evaluations of the BIC% showed 50.45 ± 9.57% for the G1 group, 55.32 ± 10.31% for the G2 group and 68.65 ± 9.98% for the G3 group, with significant statistical difference between the groups (p < 0.0001). In the BAFO% values, the G1 group presented 54.97 ± 9.56%, the G2 group 59.09 ± 10.13% and the G3 group 70.12 ± 11.07%, with statistical difference between the groups (p < 0.001). The results obtained in the evaluations show that the surface with microgrooves stimulates the process of osseointegration, accelerating the healing process, increasing the contact between the bone and the implant and the area of new bone formation