RESUMO
In this study the attention has been focused on the ester derivative of hyaluronic acid (HA), HYAFF11, as a potential three-dimensional scaffold in adipose tissue engineering. Different HYAFF11 sponges having different pore sizes, coated or not coated with HA, have been studied from a rheological and morphological point of view in order to correlate their structure to the macroscopic and degradation properties both in vitro and in vivo, using rat model. The in vitro results indicate that the HYAFF11 sponges possess proper structural and mechanical properties to be used as scaffolds for adipose tissue engineering and, among all the analysed samples, uncoated HYAFF11 large-pore sponges showed a longer lasting mechanical stability. From the in vivo results, it was observed that the elastic modulus of scaffolds seeded with preadipocytes, the biohybrid constructs, and explanted after 3 months of implantation in autologous rat model are over one order of magnitude higher than the corresponding values for the native tissue. These results could suggest that the implanted scaffolds can be invaded and populated by different cells, not only adipocytes, that can produce new matrix having different properties from that of adipose tissue.
Assuntos
Adipócitos/citologia , Materiais Revestidos Biocompatíveis/química , Ácido Hialurônico/química , Engenharia Tecidual/métodos , Adipócitos/metabolismo , Adipócitos/transplante , Animais , Biodegradação Ambiental , Adesão Celular , Técnicas de Cultura de Células , Células Cultivadas , Elasticidade , Ácido Hialurônico/análogos & derivados , Implantes Experimentais , Teste de Materiais , Microscopia Eletrônica de Varredura , Porosidade , Ratos , Reologia , Fatores de Tempo , Transplante HomólogoRESUMO
The only supernovae (SNe) to show gamma-ray bursts (GRBs) or early x-ray emission thus far are overenergetic, broad-lined type Ic SNe (hypernovae, HNe). Recently, SN 2008D has shown several unusual features: (i) weak x-ray flash (XRF), (ii) an early, narrow optical peak, (iii) disappearance of the broad lines typical of SN Ic HNe, and (iv) development of helium lines as in SNe Ib. Detailed analysis shows that SN 2008D was not a normal supernova: Its explosion energy (E approximately 6x10(51) erg) and ejected mass [ approximately 7 times the mass of the Sun (M(middle dot in circle))] are intermediate between normal SNe Ibc and HNe. We conclude that SN 2008D was originally a approximately 30 M(middle dot in circle) star. When it collapsed, a black hole formed and a weak, mildly relativistic jet was produced, which caused the XRF. SN 2008D is probably among the weakest explosions that produce relativistic jets. Inner engine activity appears to be present whenever massive stars collapse to black holes.