Formation continue: comment concilier devoir et besoins [Continuing education: how to reconcile needs and wants]

La formation continue fait à l'évidence partie intégrante de la vie du médecin, elle est non seulement un devoir éthique envers les patients mais également l'expression du besoin de se maintenir «à la page» dans sa pratique quotidienne, conséquence des progrès rapides en médecine, particulièrement en oncologie médicale. Elle peut être également source de plaisir quand il s'agit d'accroître ses connaissances. Ses règles minimales ont été définies depuis plusieurs années par la FMH qui délègue aux sociétés de disciplines son application pratique. En 2008, une révision nécessaire pour différentes raisons a facilité le calcul des crédits. Même si le total des heures de formation est resté le même (50 crédits), il a été partagé par deux : 25 pour la formation spécifique et 25 qui peuvent être acquis dans une autre discipline (révision de mars 2009 du Règlement pour la formation continue, art. 5a). Cette révision n'a pas réjoui toutes les sociétés de spécialistes qui gardent la faculté de revoir à la hausse le minimum jugé nécessaire à leur discipline. La quantité des offres de formation continue pour les médecins pose le problème d'être proprement pléthorique (congrès nationaux et internationaux, e-learning, symposiums locaux, etc.), il n'en va pas de même de leur qualité. Dans le domaine de l'oncologie médicale, les offres sont abondantes dans un contexte de marketing évident : les maisons pharmaceutiques parrainent des réunions avec un orateur mercenaire, prestigieux si possible, invité à vanter un produit spécifique dans un cycle de présentations en différents lieux de Romandie (avec à chaque fois, la possibilité d'inscrire des crédits à l'actif des participants)... Elles soutiennent également, par leur logistique, de miniconférences organisées par les différentes institutions locales et auxquelles les médecins ne participent que de façon sporadique vu leur intérêt souvent très secondaire - il n'est pas rare que l'auditoire médical se résume à cinq ou dix participants. Au final, ces offres dispersées et de qualité discutable monopolisent les ressources qui se raréfient rapidement dans le contexte économique actuel et qui doivent impérativement être utilisées de manière plus judicieuse, notamment en évitant les manifestations répétitives. Devant toutes ces offres, il est souvent difficile pour la société de discipline de séparer le bon grain de l'ivraie et en conséquence d'attribuer de manière objective les crédits de formation. Partant de ce constat, un petit groupe romand de médecins oncologues praticiens installés et des centres universitaires ont réfléchi à l'idée de regrouper au sein d'une seule structure romande l'organisation d'une formation continue qui réponde à la fois aux besoins et à l'exigence de qualité. Ses tâches sont multiples : mettre sur pied annuellement plusieurs demi-journées de formation, préaviser avec un comité scientifique de la qualité de la formation continue distillée sur son territoire de compétence (sans empiéter sur les prérogatives de la commission pour la formation postgraduée de la Société suisse d'oncologie médicale - SSOM) en rapprochant les centres universitaires, les hôpitaux cantonaux et régionaux, et les praticiens. Ainsi est née l'association FoROMe (Formation romande en oncologie médicale). Sa légitimité a été établie par la SSOM et par le Comité pour la formation postgraduée et continue (nouvellement SIWF) de la FMH. Elle est maintenant en mesure de mettre en application les tâches pour lesquelles elle a été constituée. Il est évident que cela n'ira pas sans résistance et que certains diront qu'ils ne voient pas la nécessité d'une structure supplémentaire, que les sociétés de disciplines font très bien leur travail, qu'il s'agit encore là d'une atteinte à la liberté. Cependant les nécessités économiques vont tôt ou tard venir au secours de la logique pour confirmer les changements que cette démarche a permis d'anticiper. A l'avenir, il s'agira d'assurer le bien-fondé de cette initiative et de rester vigilant au bon fonctionnement de cette structure à la satisfaction de nos membres.

Targeting mTORC2 inhibits colon cancer cell proliferation in vitro and tumor formation in vivo

The mammalian target of rapamycin (mTOR), which exists in two functionally distinct complexes, mTORC1 and mTORC2 plays an important role in tumor growth. Whereas the role of mTORC1 has been well characterized in this process, little is known about the functions of mTORC2 in cancer progression. In this study, we explored the specific role of mTORC2 in colon cancer using a short hairpin RNA expression system to silence the mTORC2-associated protein rictor. We found that downregulation of rictor in HT29 and LS174T colon cancer cells significantly reduced cell proliferation. Knockdown of rictor also resulted in a G1 arrest as observed by cell cycle analysis. We further observed that LS174T cells deficient for rictor failed to form tumors in a nude mice xenograft model. Taken together, these results show that the inhibition of mTORC2 reduces colon cancer cell proliferation in vitro and tumor xenograft formation in vivo. They also suggest that specifically targeting mTORC2 may provide a novel treatment strategy for colorectal cancer.

Old ferricrete landscape dismantling in Central Africa rain forest zone: formation of the present downslope iron accumulations.

Present downslope iron accumulations were investigated in the rainforest zone in southern Cameroon. Six clay and Fe-hydroxide dominated patterns have been identified and occur on the lower part of hill slopes. They can be subdivided in three different sequences, related to gentle, moderate or steep slopes. They are discontinuous with respect to the dismantling zone of the old ferricrete cap formed at Cretaceous period. They show a gradual development from a soft Fe-crust (carapace) to a vesicular facies that will, with time, cover the whole landscape again.

Regulatory RNA as mediator in GacA/RsmA-dependent global control of exoproduct formation in Pseudomonas fluorescens CHA0.

In Pseudomonas fluorescens CHA0, an antagonist of root-pathogenic fungi, the GacS/GacA two-component system tightly controls the expression of antifungal secondary metabolites and exoenzymes at a posttranscriptional level, involving the RNA-binding protein and global regulator of secondary metabolism RsmA. This protein was purified from P. fluorescens, and RNA bound to it was converted to cDNA, which served as a probe to isolate the corresponding chromosomal locus, rsmZ. This gene encoded a regulatory RNA of 127 nucleotides and a truncated form lacking 35 nucleotides at the 3' end. Expression of rsmZ depended on GacA, increased with increasing population density, and was stimulated by the addition of a solvent-extractable extracellular signal produced by strain CHA0 at the end of exponential growth. This signal appeared to be unrelated to N-acyl-homoserine lactones. A conserved upstream element in the rsmZ promoter, but not the stress sigma factor RpoS, was involved in rsmZ expression. Overexpression of rsmZ effectively suppressed the negative effect of gacS and gacA mutations on target genes, i.e., hcnA (for hydrogen cyanide synthase) and aprA (for the major exoprotease). Mutational inactivation of rsmZ resulted in reduced expression of these target genes in the presence of added signal. Overexpression of rsmA had a similar, albeit stronger negative effect. These results support a model in which GacA upregulates the expression of regulatory RNAs, such as RsmZ of strain CHA0, in response to a bacterial signal. By a titration effect, RsmZ may then alleviate the repressing activity of RsmA on the expression of target mRNAs.

Photometric Bgr survey of the distant clusters of galaxies CL 1613+3104 and CL 1600+4109

We present a set of photometric data concerning two distant clusters of galaxies: Cl 1613+3104 (z=0.415) and Cl 1600+4109 (z=0.540). The photometric survey extends to a field of about 4' x 3'. It was performed in 3 filters: Johnson B, and Thuan-Gunn g and r. The sample includes 679 objects in the field of Cl 1613+3104 and 334 objects in Cl 1600+4109.

New measurements of radial velocities in clusters of galaxies

Redshifts for 100 galaxies in 10 clusters of galaxies are presented based on data obtained between March 1984 and March 1985 from Calar Alto, La Palma, and ESO, and on data from Mauna Kea. Data for individual galaxies are given, and the accuracy of the velocities of the four instruments is discussed. Comparison with published data shows the present velocities to be shifted by + 4.0 km/s on average, with a standard deviation in the difference of 89.7 km/s, consistent with the rms of redshift measurements which range from 50-100 km/s.

Photometric and Spectroscopic Observations of the Cluster of Galaxies Abell 2390

Spectroscopic and photometric observations in a 6 arcmin x 6 arcmin field centered on the rich cluster of galaxies Abell 2390 are presented. The photometry concerns 700 objects and the spectroscopy 72 objects. The redshift survey shows that the mean redshift of the cluster is 0.232. An original method for automatic determination of the spectral type of galaxies is presented.

Photometric and spectroscopic survey of the cluster of galaxies Abell A2218

We present new photometric and spectroscopic observations of objects in the field of the cluster of galaxies Abell 2218. The photometric survey, centered on the cluster core, extends to a field of about 4 x 4 arcmin. It was performed in 5 bands (B,g,r,i and z filters). This sample, which includes 729 objects, is about three times larger than the survey made by Butcher and collaborators (Butcher et al., 1983, Butcher and Oemler, 1984) in the same central region of the field. Only 228 objects appear in both catalogues since our survey covers a smaller region. The spectral range covered by our filters is wider and the photometry is much deeper, up to magnitude 27 in r. The spectroscopic survey concerns 66 objects, on a field comparable to that of Butcher and collaborators. From our observations we calculate the mean redshift of the cluster, 0.1756, and its velocity dispersion, 1370 km/s. The spectral types are determined for many galaxies in the sample by comparing their spectra with synthetic ones from Rocca-Volmerange and Guiderdoni (1988).

Compatibility and ectomycorrhiza formation among Pisolithus Isolates and Eucalyptus spp

Twenty-nine isolates of the ectomycorrhiza fungus Pisolithus sp. from different geographical and host origins were tested for their ability to form ectomycorrhizae on Eucalyptus grandis and E. urophylla seedlings under greenhouse conditions. The ectomycorrhiza-forming capacity of isolates varied greatly from one eucalypt species to the other. All isolates from Eucalyptus, nine from Pinus spp. and two isolates from unknown hosts formed mycorrhizae with E. grandis and E. urophylla. Root colonization rates varied from 0 to 5.2 % for all Pinus isolates and those from unknown hosts. Colonization rates for these isolates were lower than those observed for Eucalyptus isolates (0.8 to 89.4 %). Three isolates from unknown hosts formed mycorrhizae with neither Eucalyptus species. The main characteristic for distinguishing Pinus from Eucalyptus isolates was mantle color. These data corroborate previous results obtained in our laboratory indicating that the isolates tested represent at least two distinct different species within the genus Pisolithus.

The Coordinated Radio and Infrared Survey for High-Mass Star Formation (The CORNISH Survey). I. Survey Design

We describe the motivation, design, and implementation of the CORNISH survey, an arcsecondresolution radio continuum survey of the inner galactic plane at 5 GHz using the Very Large Array (VLA). It is a blind survey coordinated with the northern SpitzerGLIMPSE I region covering 10° formation. A sensitivity around 2 mJy will allow the automatic distinction between radio-loud and radio-quiet midIR sources found in the Spitzersurveys. This survey has many legacy applications beyond star formation, including evolved stars, active stars and binaries, and extragalactic sources. The CORNISH survey for compact ionized sources complements other Galactic plane surveys that target diffuse and nonthermal sources, as well as atomic and molecular phases to build up a complete picture of the interstellar medium in the Galaxy.