3XMM J185246.6+003317: another low magnetic field magnetar

We study the outburst of the newly discovered X-ray transient 3XMMJ185246.6+003317, re-analyzing all available XMM-Newton observations of the source to perform a phase-coherent timing analysis, and derive updated values of the period and period derivative. We find the source rotating at P = 11.55871346(6) s (90% confidence level; at epoch MJD 54728.7) but no evidence for a period derivative in the seven months of outburst decay spanned by the observations. This translates to a 3σ upper limit for the period derivative of ˙ P <1.4×10−13 s s−1, which, assuming the classical magneto-dipolar braking model, gives a limit on the dipolar magnetic field of Bdip < 4.1×1013 G. The X-ray outburst and spectral characteristics of 3XMM J185246.6+003317 confirm its identification as a magnetar, but the magnetic field upper limit we derive defines it as the third “low-B” magnetar discovered in the past 3 yr, after SGR 0418+5729 and Swift J1822.3−1606. We have also obtained an upper limit to the quiescent luminosity (<4×1033 erg s−1), in line with the expectations for an old magnetar. The discovery of this new low field magnetar reaffirms the prediction of about one outburst per year from the hidden population of aged magnetars.

Astrophysical parameters of the peculiar X-ray transient IGR J11215−5952

Context. The current generation of X-ray satellites has discovered many new X-ray sources that are difficult to classify within the well-described subclasses. The hard X-ray source IGR J11215−5952 is a peculiar transient, displaying very short X-ray outbursts every 165 days. Aims. To characterise the source, we obtained high-resolution spectra of the optical counterpart, HD 306414, at different epochs, spanning a total of three months, before and around the 2007 February outburst with the combined aims of deriving its astrophysical parameters and searching for orbital modulation. Methods. We fit model atmospheres generated with the fastwind code to the spectrum, and used the interstellar lines in the spectrum to estimate its distance. We also cross-correlated each individual spectrum to the best-fit model to derive radial velocities. Results. From its spectral features, we classify HD 306414 as B0.5 Ia. From the model fit, we find Teff ≈ 24 700 K and log g ≈ 2.7, in good agreement with the morphological classification. Using the interstellar lines in its spectrum, we estimate a distance to HD 306414 d ≳ 7 kpc. Assuming this distance, we derive R∗ ≈ 40 R⊙ and Mspect ≈ 30 M⊙ (consistent, within errors, with Mevol ≈ 38 M⊙, and in good agreement with calibrations for the spectral type). Analysis of the radial velocity curve reveals that radial velocity changes are not dominated by the orbital motion, and provide an upper limit on the semi-amplitude for the optical component Kopt ≲ 11 ± 6 km   s-1. Large variations in the depth and shape of photospheric lines suggest the presence of strong pulsations, which may be the main cause of the radial velocity changes. Very significant variations, uncorrelated with those of the photospheric lines are seen in the shape and position of the Hα emission feature around the time of the X-ray outburst, but large excursions are also observed at other times. Conclusions. HD 306414 is a normal B0.5 Ia supergiant. Its radial velocity curve is dominated by an effect that is different from binary motion, and is most likely stellar pulsations. The data available suggest that the X-ray outbursts are caused by the close passage of the neutron star in a very eccentric orbit, perhaps leading to localised mass outflow.

Pulse phase-coherent timing and spectroscopy of CXOU J164710.2−45521 outbursts

We present a long-term phase-coherent timing analysis and pulse-phase resolved spectroscopy for the two outbursts observed from the transient anomalous X-ray pulsar CXOU J164710.2−455216. For the first outburst we used 11 Chandra and XMM–Newton observations between 2006 September and 2009 August, the longest baseline yet for this source. We obtain a coherent timing solution with P = 10.61065583(4) s, Ṗ = 9.72(1) × 10−13 s s−1 and P̈ = –1.05(5) × 10−20 s s−2. Under the standard assumptions this implies a surface dipolar magnetic field of ∼1014 G, confirming this source as a standard B magnetar. We also study the evolution of the pulse profile (shape, intensity and pulsed fraction) as a function of time and energy. Using the phase-coherent timing solution we perform a phase-resolved spectroscopy analysis, following the spectral evolution of pulse-phase features, which hints at the physical processes taking place on the star. The results are discussed from the perspective of magnetothermal evolution models and the untwisting magnetosphere model. Finally, we present similar analysis for the second, less intense, 2011 outburst. For the timing analysis we used Swift data together with 2 XMM–Newton and Chandra pointings. The results inferred for both outbursts are compared and briefly discussed in a more general framework.

Modelling of the surface emission of the low magnetic field magnetar SGR 0418+5729

We perform a detailed modelling of the post-outburst surface emission of the low magnetic field magnetar SGR 0418+5729. The dipolar magnetic field of this source, B=6×1012G estimated from its spin-down rate, is in the observed range of magnetic fields for normal pulsars. The source is further characterized by a high pulse fraction and a single-peak profile. Using synthetic temperature distribution profiles, and fully accounting for the general-relativistic effects of light deflection and gravitational redshift, we generate synthetic X-ray spectra and pulse profiles that we fit to the observations. We find that asymmetric and symmetric surface temperature distributions can reproduce equally well the observed pulse profiles and spectra of SGR 0418. None the less, the modelling allows us to place constraints on the system geometry (i.e. the angles ψ and ξ that the rotation axis makes with the line of sight and the dipolar axis, respectively), as well as on the spot size and temperature contrast on the neutron star surface. After performing an analysis iterating between the pulse profile and spectra, as done in similar previous works, we further employed, for the first time in this context, a Markov-Chain Monte Carlo approach to extract constraints on the model parameters from the pulse profiles and spectra, simultaneously. We find that, to reproduce the observed spectrum and flux modulation: (a) the angles must be restricted to 65° ≲ ψ + ξ ≲ 125° or 235° ≲ ψ + ξ ≲ 295°; (b) the temperature contrast between the poles and the equator must be at least a factor of ∼6, and (c) the size of the hottest region ranges between 0.2 and 0.7 km (including uncertainties on the source distance). Lastly, we interpret our findings within the context of internal and external heating models.

Towards Explaining Anti-Foreign Violence in Germany. CES Germany & Europe Working Papers, No. 04.8 (Series 53), 1993

Gennany has recently witnessed a vast increase in anti-foreign violence. Assembling data from a wide variety of recent research, the paper addresses two basic questions: to what extent is the outburst of xenophobic attacks a German peculiarity? and what are the explanations for the mcreasing violence? An analysis of criminal statistics of various European countries and of comparative opinion polls in the European Community shows that Germany has indeed witnessed a growth of anti-foreign sentiment, and a level of violence that is conspicuous from a com­ parative perspective. Four possible determinants of this peculiarity of recent German history are discussed: (1) the growing ethnic and cultural heterogeneity due to the vast increase in immigration from non-European countries; (2) the increasing costs of foreigners' claims on the German welfare state; (3) the economic context of immigration; and (4) the transformation of national identity in the context of German unification. It is shown that neither the rate of immigration nor the position of foreigners in the German welfare state yields satisfactory explanations for the recent upsurge in violence, which only occurred after unification. The key for an explanation lies in a particu­lar macro-constellation that is characterized by the concurrence of a massive wave of immigration with an economic crisis, and with the ethnicization of German national identity in the context of unification. Anti-foreign sentiments do not automatically follow increases in immigration, but grow in a specific political climate to which the political elites actively contribute.

Morocco’s illiberal regime and fragmented political society. Arab Citizenship Review No. 10, October 2015

The post-Arab Spring period in Morocco has undergone different stages of changing state-society relations with regard to democracy, citizenship and human rights. The first stage, between February 2011 and the summer of 2013, was characterised by popular protests demanding democracy and freedom. People criticised public policies related to civil, political and social rights (employment, health, education, the status of women, and the issue of Amazigh). This outburst put the state in an awkward, defensive position. If we compare Morocco with the other Arab Spring countries, the Moroccan state’s reaction was moderate in its use of violence and repression, and it was positive, in that it resulted in the implicit, yet official acceptance of the demands for democracy, citizenship and battling corruption. In his speech on 9 March 2011, the king pledged to modify the Constitution and democratise the institutions.

Geochemistry of sediment core PS2456-4

Sediment core PS2458 from the Laptev Sea continental margin (983-m water depth) stems from a position close to the paleoriver mouth of Lena and Yana rivers. It was dated by AMS-14C and analyzed in high resolution for oxygen isotopes of planktic foraminifers. Except the uppermost 100 cm and possibly the lowermost meter of the 8-m-long core, the sediments were deposited during the last deglaciation (14.5-8.0 cal-ka). According to 210Pb data, the uppermost 100 cm represents only the last 200 years. Planktic foraminifers are present throughout the dated deglacial interval, with the exception of a short time after ca. 13 cal-ka. Taking into account the global "ice volume effect" on the oxygen isotopic composition of the foraminifers, the isotopic record is considered to reflect salinity changes which were influenced by variable freshwater runoff and a growing marine influence during the postglacial transgression of the Laptev Sea shelf. The most conspicuous feature in the isotopic record is an outstanding peak dated to ca. 13 cal-ka. It is proposed that it represents a rapid outburst of large amounts of freshwater, possibly from an ice-dammed lake in the hinterland. Possible correlations to the onset of the cool Younger Dryas event in the northern hemisphere are discussed.

Avaliação das coroas dos primeiros e terceiros molares superiores, nos tratamentos com extrações de segundos molares superiores

A presente pesquisa teve como objetivo avaliar, por meio de modelos de gesso, a posição das coroas dos primeiros e terceiros molares superiores permanentes, após a irrupção espontânea dos terceiros molares, na posição dos segundos molares extraídos com finalidade ortodôntica, comparando-os com as coroas dos primeiros e segundos molares superiores permanentes de uma amostra de oclusão normal natural. A amostra experimental constituiu-se de 25 indivíduos, leucodermas, com idade média no início do tratamento de 15,6 anos, sendo 17 do sexo feminino e 8 do sexo masculino, tratados com extrações de segundos molares superiores. A amostra controle constituiu-se de 60 indivíduos do sexo masculino e sexo feminino, com idade média de 15,6 anos e faixa etária compreendida entre 12 e 21 anos, que apresentavam oclusão normal. Foram avaliadas as angulações, as inclinações e as distâncias mésio-distais das coroas dentárias dos terceiros molares e primeiros molares do grupo tratado e dos segundos molares e primeiros molares do grupo controle ou normal. Foram, também, verificadas as diferenças de alturas entre as coroas dentárias dos dois grupos. Verificou-se que nos casos tratados os valores médios das angulações mésio-distais e das inclinações vestíbulo-linguais das coroas dos terceiros molares superiores e dos primeiros molares superiores foram estatisticamente diferentes dos valores médios das angulações mésio-distais e das inclinações vestíbulo-linguais das coroas dos segundos molares superiores e dos primeiros molares superiores na amostra de oclusão normal natural. Observou-se que somente as distâncias mésio-distais das coroas dos terceiros molares superiores mostraram ser significativamente menores que as coroas dos segundos molares superiores da amostra de oclusão normal natural, tanto para o sexo feminino quanto para o masculino. O valor médio da diferença de altura entre as coroas dos primeiros molares e terceiros molares do grupo experimental e das coroas dos primeiros molares e segundos molares do grupo controle foi de 1,11mm, não havendo diferença entre os grupos. Ocorreu a presença de dimorfismo sexual nos valores da distância mésio-distais das coroas dentárias dos primeiros molares superiores do grupo controle e experimental, na distância mésio-distal das coroas dentárias dos segundos molares superiores do grupo controle e na inclinação vestíbulo-linguais das coroas dos terceiros molares superiores do grupo experimental. Nas demais avaliações não houve dimorfismo sexual.

Dynamics and topographic organization of recursive self-organizing maps

Recently there has been an outburst of interest in extending topographic maps of vectorial data to more general data structures, such as sequences or trees. However, there is no general consensus as to how best to process sequences using topographicmaps, and this topic remains an active focus of neurocomputational research. The representational capabilities and internal representations of the models are not well understood. Here, we rigorously analyze a generalization of the self-organizingmap (SOM) for processing sequential data, recursive SOM (RecSOM) (Voegtlin, 2002), as a nonautonomous dynamical system consisting of a set of fixed input maps. We argue that contractive fixed-input maps are likely to produce Markovian organizations of receptive fields on the RecSOM map. We derive bounds on parameter β (weighting the importance of importing past information when processing sequences) under which contractiveness of the fixed-input maps is guaranteed. Some generalizations of SOM contain a dynamic module responsible for processing temporal contexts as an integral part of the model. We show that Markovian topographic maps of sequential data can be produced using a simple fixed (nonadaptable) dynamic module externally feeding a standard topographic model designed to process static vectorial data of fixed dimensionality (e.g., SOM). However, by allowing trainable feedback connections, one can obtain Markovian maps with superior memory depth and topography preservation. We elaborate on the importance of non-Markovian organizations in topographic maps of sequential data. © 2006 Massachusetts Institute of Technology.

Buborékok és legendák. Válságok és válságmagyarázatok - a tulipánmánia és a Déltengeri Társaság, I. rész (Bubbles and myths, crises and explanations: tulip mania and the South Sea bubble. I.)

A 2007 óta kibontakozó válság újból divatba hozta a korai buborékok és válságok témáját. A jelenlegi válság nyomán újraéledtek a makroökónómiai viták, kétségessé vált a "nagy mérséklődés" és az újklasszikus szintézis érvényessége. Az 1634-1637 közötti holland tulipánmánia - mint az első buborék - sokféle értelmezése ismeretes: a tömeghisztéria kitörésétől a hatékony pénzügyi piacok korai példáján át a kulturális sokkig. Áttekintve ezeket, a cikk visszavezeti a tulipánmánia közismert anekdotikus leírásait az eredeti forrásokig, és megmutatja, milyen módon és céllal használták fel ezeket a közgazdászok és történészek saját elemzéseikben. / === / The accounts of early bubbles and crises are becoming fashionable again in economic discourse during the recent downturn. The article, having looked at the revival of macroeconomic debate provoked by the failure of current theory, sums up various interpretations of the Dutch tulip mania of 1634-7. These range from an outburst of popular madness, through an early example of an efficient financial market, to an instance of culture shock. Some well-known anecdotes about tulip mania are traced back to their original sources, and the article explores the various patterns and intentions in the use economists and historians have made of them.

Imaginários da morte: poética das imagens em cemitérios brasileiros

The thesis presented is committed to a poetic reading that results in the creation of meaning and images of the death from the various cultural practices and symbolic representations exposed in urban cemeteries in some Brazilian cities, aiming to give visibility to new understandings about the imaginary of the in the contemporary scene. Death, therefore, will be seen as a imagining condition of anthroposwhen starts itself from the prerogative of the human consciousness of death (MORIN, 1970), in other words, this awareness that man has he will die and that triggers reflections about their existence allows the emergence of a number of practices such as: mourning, funeral rituals and the creation of several impregnated representations of human emotions emerged from the death facing the man and present, in a more evident form in cemeterial spaces. For this, it focuses on the conflictuous dimension that man establishes with death, because the cultural practices and symbolic representations observed in the research field are the result of this conflict and allow the expansion of the senses about this issue, to the extent that these are coated with a fantastic aura, mystical, secret, spooky, fearful, religious, building a complex imagination. The general plan of this study is to discuss and create, from a phenomenology of imagination and materials / dynamics imagination, as well as along the lines treated by Gaston Bachelard, images of death, from a field experience in cemeteries in Brazil. For this, it is assumed, to observe the cultural practices and symbolic representations in these spaces, a posture able to make the experience into the search field a moment of symbolic exchanges and creation. Thus, it was used observation, conversations with visitors and employees of the cemeteries and the capture of photographic records. The data produced as a fragment of a conversation, a tearful outburst about the loss of a relative, a melancholic epitaph, a flower on the grave or a cry captured by photography were seen as detonators of meanings and a poetic of the imagination.