Occupational choice and development

The rise in world trade since 1970 has been accompanied by a rise in the geographic span of control of management and, hence, also a rise in the e ective international mobility of labor services. We study the e ect of such a globalization of the world's labor markets. The world's welfare gains depend positively on the skill-heterogeneity of the world's labor force. We nd that when peoplecan choose between wage work and managerial work, the worldwide labor market raises output by more in the rich and the poor countries, and by less in the middle-income countries. This is because the middle-income countries experience the smallest change in the factor-price ratio, and where the option to choose between wage work and managerial work has the least value in the integratedeconomy. Our theory also establishes that after economic integration, the high skill countries see a disproportionate increase in managerial occupations. Using aggregate data on GDP, openness and occupations from 115 countries, we find evidence for these patterns of occupational choice.

On forward induction and evolutionary and strategic stability

We analyze which normal form solution concepts capture the notion offorward induction, as defined by van Damme (JET, 1989) in the classof generic two player normal form games preceded by an outsideoption. We find that none of the known strategic stability concepts(including Mertens stable sets and hyperstable sets) captures this form of forward induction. On the other hand, we show that the evolutionary concept of EES set (Swinkels, JET, 1992) is always consistent with forward induction.

Neurologie et voyages

Le mal de voyage, l'insomnie, les troubles du sommeil, la fatigue, le jet-lag et des troubles sensitifs transitoires sont des symptômes très fréquents lors des voyages et pour la plupart banals. Les maladies neurologiques déclenchées ou causées par le voyage sont rares et incluent des accidents vasculaires cérébraux (AVC) liés aux emboles paradoxaux après un voyage prolongé en avion, des crises d'épilepsie ou des troubles du sommeil déclenchés par le décalage horaire, des symptômes de décompression lors de la plongée ou montée en altitude. Dans cet article sont aussi discutées les maladies liées à la haute altitude(céphalée de haute altitude, mal aigu des montagnes), des troubles neurologiques liés à la déshydratation et à la chaleur ainsi que les infections acquises lors de voyages.

Electromagnetic radiation initiated by hadronic jets from microquasars in the ISM

Microquasars are potential candidates to produce a non-negligible fraction of the observed galactic cosmic rays. The protons accelerated at the jet termination shock interact with the interstellar medium and may produce detectable fluxes of extended emission at different energy bands: high-energy and very high-energy gamma-rays produced by neutral pion-decay, synchrotron and bremsstrahlung emission in a wide energy range generated by the secondary electrons produced by charged pion-decay. We discuss the association between this scenario and some of the unidentified EGRET sources in the galactic plane.

A numerical model for the gamma-ray emission of the microquasar LS 5039

The possible association between the microquasar LS 5039 and the EGRET source 3EG J1824-1514 suggests that microquasars could also be sources of high energy gamma-rays. In this paper, we explore, with a detailed numerical model, if this system can produce the emission detected by EGRET (>100 MeV) through inverse Compton (IC) scattering. Our numerical approach considers a population of relativistic electrons entrained in a cylindrical inhomogeneous jet, interacting with both the radiation and the magnetic fields, taking into account the Thomson and Klein-Nishina regimes of interaction. The computed spectrum reproduces the observed spectral characteristics at very high energy.

A search for microquasar candidates at low galactic latitudes

Recent studies of relativistic jet sources in the Galaxy, also known as microquasars, have been very useful in trying to understand the accretion/ejection processes that take place near compact objects. However, the number of sources involved in such studies is still small. In an attempt to increase the number of known microquasars we have carried out a search for new Radio Emitting X-ray Binaries (REXBs). These sources are the ones to be observed later with VLBI techniques to unveil their possible microquasar nature. To this end, we have performed a cross-identification between the X-ray ROSAT all sky survey Bright Source Catalog (RBSC) and the radio NRAO VLA Sky Survey (NVSS) catalogs under very restrictive selection criteria for sources with |b|<5 degrees. We have also conducted a deep observational radio and optical study for six of the selected candidates. At the end of this process two of the candidates appear to be promising, and deserve additional observations aimed to confirm their proposed microquasar nature.

The extraordinarily bright optical afterglow of GRB 991208 and its host galaxy

Observations of the extraordinarily bright optical afterglow (OA) of GRB 991208 started 2.1 d after the event. The flux decay constant of the OA in the R-band is -2.30 +/- 0.07 up to 5 d, which is very likely due to the jet effect, and after that it is followed by a much steeper decay with constant -3.2 +/- 0.2, the fastest one ever seen in a GRB OA. A negative detection in several all-sky films taken simultaneously to the event implies either a previous additional break prior to 2 d after the occurrence of the GRB (as expected from the jet effect). The existence of a second break might indicate a steepening in the electron spectrum or the superposition of two events. Once the afterglow emission vanished, contribution of a bright underlying SN is found, but the light curve is not sufficiently well sampled to rule out a dust echo explanation. Our determination of z = 0.706 indicates that GRB 991208 is at 3.7 Gpc, implying an isotropic energy release of 1.15 x 10E53 erg which may be relaxed by beaming by a factor > 100. Precise astrometry indicates that the GRB coincides within 0.2' with the host galaxy, thus given support to a massive star origin. The absolute magnitude is M_B = -18.2, well below the knee of the galaxy luminosity function and we derive a star-forming rate of 11.5 +/- 7.1 Mo/yr. The quasi-simultaneous broad-band photometric spectral energy distribution of the afterglow is determined 3.5 day after the burst (Dec 12.0) implying a cooling frequency below the optical band, i.e. supporting a jet model with p = -2.30 as the index of the power-law electron distribution.

High-energy gamma-ray emission from microquasars: LS 5039 and LS I+61303

The possible associations between the microquasars LS 5039 and LS I +61 303 and the EGRET sources 3EG J1824-1514 and 3EG J0241+6103 suggest that microquasars could also be sources of high-energy gamma-rays. In this work, we present a detailed numerical inverse Compton (IC) model, based on a microquasar scenario, that reproduces the high-energy gamma-ray spectra and variability observed by EGRET for the mentioned sources. Our model considers a population of relativistic electrons entrained in a cylindrical inhomogeneous jet that interact through IC scattering with both the radiation and the magnetic fields.

Leptonic secondary emission in a hadronic microquasar model

Context.It has been proposed that the origin of the very high-energy photons emitted from high-mass X-ray binaries with jet-like features, so-called microquasars (MQs), is related to hadronic interactions between relativistic protons in the jet and cold protons of the stellar wind. Leptonic secondary emission should be calculated in a complete hadronic model that includes the effects of pairs from charged pion decays inside the jets and the emission from pairs generated by gamma-ray absorption in the photosphere of the system. Aims.We aim at predicting the broadband spectrum from a general hadronic microquasar model, taking into account the emission from secondaries created by charged pion decay inside the jet. Methods.The particle energy distribution for secondary leptons injected along the jets is consistently derived taking the energy losses into account. The spectral energy distribution resulting from these leptons is calculated after assuming different values of the magnetic field inside the jets. We also compute the spectrum of the gamma-rays produced by neutral pion-decay and processed by electromagnetic cascades under the stellar photon field. Results.We show that the secondary emission can dominate the spectral energy distribution at low energies (~1 MeV). At high energies, the production spectrum can be significantly distorted by the effect of electromagnetic cascades. These effects are phase-dependent, and some variability modulated by the orbital period is predicted.

INTEGRAL and XMM-Newton observations towards the unidentified MeV source GRO J1411-64.

The COMPTEL unidentified source GRO J1411-64 was observed by INTEGRAL, and its central part, also by XMM-Newton. The data analysis shows no hint for new detections at hard X-rays. The upper limits in flux herein presented constrain the energy spectrum of whatever was producing GRO J1411-64, imposing, in the framework of earlier COMPTEL observations, the existence of a peak in power output located somewhere between 300-700 keV for the so-called low state. The Circinus Galaxy is the only source detected within the 4$\sigma$ location error of GRO J1411-64, but can be safely excluded as the possible counterpart: the extrapolation of the energy spectrum is well below the one for GRO J1411-64 at MeV energies. 22 significant sources (likelihood $> 10$) were extracted and analyzed from XMM-Newton data. Only one of these sources, XMMU J141255.6-635932, is spectrally compatible with GRO J1411-64 although the fact the soft X-ray observations do not cover the full extent of the COMPTEL source position uncertainty make an association hard to quantify and thus risky. The unique peak of the power output at high energies (hard X-rays and gamma-rays) resembles that found in the SED seen in blazars or microquasars. However, an analysis using a microquasar model consisting on a magnetized conical jet filled with relativistic electrons which radiate through synchrotron and inverse Compton scattering with star, disk, corona and synchrotron photons shows that it is hard to comply with all observational constrains. This and the non-detection at hard X-rays introduce an a-posteriori question mark upon the physical reality of this source, which is discussed in some detail.

Possible hot spots excited by the relativistic jets of Cygnus X-3

We present the results of a deep search for associated radio features in the vicinity of the microquasar Cygnus X-3. The motivation behind is to find out evidence for interaction between its relativistic jets and the surrounding interstellar medium, which could eventually allow us to perform calorimetry of the total energy released by this microquasar during its flaring lifetime. Remarkably, two radio sources with mJy emission level at centimeter wavelengths have been detected in excellent alignment with the position angle of the inner radio jets. We propose that these objects could be the hot spots where the relativitic outflow collides with the ambient gas in analogy with Fanaroff-Riley II radio galaxies. These candidate hot spots are within a few arc-minutes of Cygnus X-3 and, if physically related, the full linear extent of the jet would reach tens of parsecs. We discuss here the evidence currently available to support this hypothesis based on both archival data and our own observations.

Time-resolved imaging of the laser forward transfer of liquids

Time-resolved imaging is carried out to study the dynamics of the laser-induced forward transfer of an aqueous solution at different laser fluences. The transfer mechanisms are elucidated, and directly correlated with the material deposited at the analyzed irradiation conditions. It is found that there exists a fluence range in which regular and well-defined droplets are deposited. In this case, laser pulse energy absorption results in the formation of a plasma, which expansion originates a cavitation bubble in the liquid. After the further expansion and collapse of the bubble, a long and uniform jet is developed, which advances at a constant velocity until it reaches the receptor substrate. On the other hand, for lower fluences no material is deposited. In this case, although a jet can be also generated, it recoils before reaching the substrate. For higher fluences, splashing is observed on the receptor substrate due to the bursting of the cavitation bubble. Finally, a discussion of the possible mechanisms which lead to such singular dynamics is also provided.

SEPT4, a p53 target gene product, implicates p 53 in the regulation of exocytosis

Résumé : Le cancer, qui est responsable d'un quart des décès en Suisse, exhibe un état cellulaire désordonné, qui lui-même, est la conséquence d'un dérèglement des gènes. Le gène le plus fréquemment altéré, dans les cas de cancers humains, est p53. Ce gène encode un facteur de transcription, impliqué dans la régulation de nombreux gènes impliqués dans le cycle cellulaire, l'apoptose ou la différenciation. Notre laboratoire a récemment identifié seize nouveaux gènes, dont l'expression est régulée par p53, parmi lesquels sept4, su jet de cette thèse. La protéine 5EPT4 appartient à la famille des septines, qui est impliquée dans la cytokinèse. Dans ce travail, nous avons confirmé la régulation de l'expression de sept4 par p53 dans des tissus de souris, et étonnamment, seul un des deux promoteurs du gène sept4 est contrôlé par p53. En outre, l'approche immunohistologique nous a permis de supposer une implication de la protéine SEPT4 dans le mécanisme de l'exocytose. Cette hypothèse a été confirmée par l'interaction de SEPT4 avec la protéine syntaxine 1A, et par son activité inhibitrice sur la sécrétion stimulée. En élargissant l'étude de la protéine SEPT4, nous avons découvert que celle-ci avait comme partenaire fonctionnel, la protéine Pinl, une enzyme qui catalyse l'isomérisation cis-trans du lien peptidique précédant une proline. bans ce contexte, nous avons démontré que l'interaction entre ces deux protéines reposait sur le domaine WW de Pinl, un type de domaine reconnaissant les motifs phosphoséryl-prolyl et phosphothréonyl-prolyl. Ce dernier résultat nous a conduit à examiner la phosphorylation de 5EPT4. Nous avons démontré que la partie N-terminale de SEPT4 était phosphorylée par la kinase Cdk5. La co¬expression de Cdk5 et de SEPT4 stimule la dégradation de SEPT4, indépendamment de la voie du protéasome. Ainsi, l'ensemble de nos observations fournissent l'évidence de l'engagement de la protéine SEPT4 dans la régulation de l'exocytose, et soutiennent le rôle de p53 dans le contrôle de l'exocytose, via SEPT4, ce qui constituerait un nouveau rôle fonctionnel pour ce gardien du génome. Summary: Cancer, which is responsible for a quarter of the deaths in Switzerland, exhibits a disordered cellular state, which itself, is the consequence of an altered state of genes. The most frequently altered gene in human cancer is p53. This gene encodes a transcription factor, implicated in the regulation of numerous genes involved in cell cycle, apoptosis or differentiation. Our laboratory has recently identified sixteen new genes whose expression is regulated by p53, amongst them septin 4, which is the subject of this thesis. The SEPT4 protein belongs to the septin family which is implicated in cytokinesis. In the present work, we have confirmed the regulation of sept4 expression by p53 in mouse tissues, and surprisingly, only one of the two sept4 promoters is regulated by p53. In addition, the immunohistologic approach enabled us to suppose a role of SEPT4 in exocytosis. This assumption was confirmed by the interaction of SEPT4 with syntaxin 1A, and by its inhibiting activity on stimulated secretion. By widening the analysis of SEPT4, we identified Pin1 as an interacting protein. Pin1 is an enzyme which catalyzes the cis-trans isomerization of the peptide bond preceding a proline residue. In this context, we showed that the interaction between these two proteins depends on the WW domain of Pin 1. This domain has been shown to function as a phosphoserine- or phosphothreonine¬binding module. This last result prompted us to examine phosphorylation of SEPT4. We demonstrated that the N-terminal portion of SEPT4 was phosphorylated by the Cdk5 kinase. The co-expression of Cdk5 with 5EPT4 stimulates SEPT4 degradation, independently of the proteasome pathway. Thus, these observations provide evidence for the engagement of SEPT4 in the regulation of exocytosis, and supports the role of p53 in the control of exocytosis, via SEPT4, which constitutes a new functional role for this guardian of the genome.