Actualización bibliográfica sobre el uso de preparaciones ricas en plaquetas en la cicatrización de heridas Updated review of the use of platelet rich preparations in wound healing

Las plaquetas poseen más de 20 factores de crecimiento en sus gránulos. Su secreción promueve la reparación de heridas. La cicatrización es un intrincado proceso en el cual intervienen no solo los factores plaquetarios proangiogénicos sino también factores antiangiogénicos. La preservación por congelación de las plaquetas empleada para su preservación, desestabiliza y activa la membrana plaquetaria alterando sus propiedades. En el campo del tratamiento de heridas recalcitrantes en pacientes debilitados o con enfermedades crónicas, el uso de preparaciones plaquetarias en forma de plasma fresco congelado, las preparaciones plaquetarias sonicadas, las preparaciones congeladas y deshidratadas y el uso de fragmentos de dermis alogénica, confiere efectos beneficiosos, logrando mejores tiempos de cierre en las heridas y menor alteración de la morfología de la cicatriz final. En el presente artículo, describiremos los estudios que han demostrado estos efectos, así como las encrucijadas actuales y los estudios que debemos esperar en un futuro no lejano.Platelets store more than 20 growth factors in their granules. Their secretion promotes wound healing and repair. The intricate wound healing process involves not only the angiogenic platelet factors but also de anti-angiogenic ones. The process of platelet preservation, such as freezing, disrupt the platelet membrane structure and their angiogenic properties causing platelet activation. In the field of wound healing and the management of recalcitrant wounds in debilitated and chronically ill patients, there have been several studies. These studies have focused on the use of the different platelet preparations such as fresh frozen plasma, frozen-dried platelet rich plasma, sonicated platelet rich plasma and the use of alogenic acelular dermis. Platelet preparations posses positive effects on wound healing with little alterations of the final scar tissue. In this article we will describe and discuss the studies that have involved the use of these platelet rich preparations in the filed of wound healing and we will also state the road blocks and the studies that will come in the near future regarding the use of platelets products in the field wound healing

Multi-messenger Observations of a Binary Neutron Star Merger

International audienceOn 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of $\sim 1.7\,{\rm{s}}$ with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg(2) at a luminosity distance of ${40}_{-8}^{+8}$ Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 $\,{M}_{\odot }$. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at $\sim 40\,{\rm{Mpc}}$) less than 11 hours after the merger by the One-Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ∼10 days. Following early non-detections, X-ray and radio emission were discovered at the transient’s position $\sim 9$ and $\sim 16$ days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC 4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta