Aberrant c-MET activation impairs perinuclear actin cap organization with YAP1 cytosolic relocation

Growing evidence indicates that cell and nuclear deformability plays a crucial role in the determination of cancer cells tumorigenic and metastatic potential. The perinuclear actin cap, by wrapping the nucleus with a functional network of actomyosin cables, can modulate nuclear architecture and consequently cell/nuclear elasticity. The hepatocyte growth factor receptor (MET) stands out among other membrane receptors as crucial player of the actin filaments organization, but no data are available on a specific role for MET in the actin cap assembly and the overall nuclear architecture organization. In a cell system characterized by MET hyperactivation, we observed a strong rearrangement of the cellular actin caps, with a complete dismantling of apical stress fibers and a strikingly enhanced nuclear height. CRISPR/Cas9 silencing of MET completely reverted the aberrant phenotype, resulting in flattened cells with perfectly aligned perinuclear actomyosin bundles, as well as decreased MAPK and PI3K/AKT signaling, cell proliferation rate and aggressiveness. Interestingly, MET ablated cells acquired a remarkably directed and polarized migratory phenotype, contrarily to cells with MET sustained activation showing meandering random walk. A pathway enrichment analysis comparing MET-activated and MET-KO cells RNAseq data, unveiled the contribution of multiple pathways associated with cytoskeleton remodeling, regulation of cell shape and response to mechanical stimuli. In line, the co-transcriptional activator YAP1, playing a major role in cell mechanosensing and focal adhesions/actin stabilization, appeared the culprit of the genetic reassembling of KO cells. Indeed, MET silencing was shown to induce YAP1 nuclear shuttling and increased co-transcriptional activity. Finally, we were able to induce in a normal epithelial model a phenotype closer to MET activated cancer cells only by introducing a constitutive fusion protein of MET. Taken together, our results demonstrate a new mechanism of MET-mediated actin remodeling responsible for a tumor-initiating capacity and meandering random migration, which requires YAP1 inactivation.

Stellar Relics of the hierarchical assembly of the Galaxy

This PhD Thesis is part of a long-term wide research project, carried out by the "Osservatorio Astronomico di Bologna (INAF-OABO)", that has as primary goal the comprehension and reconstruction of formation mechanism of galaxies and their evolution history. There is now substantial evidence, both from theoretical and observational point of view, in favor of the hypothesis that the halo of our Galaxy has been at least partially, built up by the progressive accretion of small fragments, similar in nature to the present day dwarf galaxies of the Local Group. In this context, the photometric and spectroscopic study of systems which populate the halo of our Galaxy (i.e. dwarf spheroidal galaxy, tidal streams, massive globular cluster, etc) permits to discover, not only the origin and behaviour of these systems, but also the structure of our Galactic halo, combined with its formation history. In fact, the study of the population of these objects and also of their chemical compositions, age, metallicities and velocity dispersion, permit us not only an improvement in the understanding of the mechanisms that govern the Galactic formation, but also a valid indirect test for cosmological model itself. Specifically, in this Thesis we provided a complete characterization of the tidal Stream of the Sagittarius dwarf spheroidal galaxy, that is the most striking example of the process of tidal disruption and accretion of a dwarf satellite in to our Galaxy. Using Red Clump stars, extracted from the catalogue of the Sloan Digital Sky Survey (SDSS) we obtained an estimate of the distance, the depth along the line of sight and of the number density for each detected portion of the Stream (and more in general for each detected structure along our line of sight). Moreover comparing the relative number (i.e. the ratio) of Blue Horizontal Branch stars and Red Clump stars (the two features are tracers of different age/different metallicity populations) in the main body of the galaxy and in the Stream, in order to verify the presence of an age-metallicity gradient along the Stream. We also report the detection of a population of Red Clump stars probably associated with the recently discovered Bootes III stellar system. Finally, we also present the results of a survey of radial velocities over a wide region, extending from r ~ 10' out to r ~ 80' within the massive star cluster Omega Centauri. The survey was performed with FLAMES@VLT, to study the velocity dispersion profile in the outer regions of this stellar system. All the results presented in this Thesis, have already been published in refeered journals.