Multi-messenger observations of a binary neutron star merger

On 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 ~1.7 s with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg2 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 Mo. 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 ~40 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 ~9 and ~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 NGC4993 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

Effects of the use of MIG3 bioceramics fabrics use - long infrared emitter - in pain, intolerance to cold and periodic limb movements in post-polio syndrome Efeitos do uso de tecidos com biocerâmica MIG3 - emissora de infravermelho longo - na dor, intolerância ao frio e movimentos periódicos dos membros na síndrome pós-poliomielite

The main post-polio syndrome (PPS) symptoms are new-onset weakness, new-onset atrophy, fatigue, cold intolerance, and pain associated with sleep disturbances. The polysomnographic study is the gold pattern to analyze sleep disorders. OBJECTIVE: To assess pain, intolerance to cold and periodic limb movements (PLM) index before and after the use of MIG3 bioceramic fabrics over 4 weeks. METHOD: 12 patients with PPS from UNIFESP/EPM. All patients were submitted to polysomnography and infra-red examinations with answered scales of pain and intolerance to cold before and after the use of MIG3 bioceramics fabrics. RESULTS: There were significant decreases in pain and PLM index. CONCLUSION: MIG3 bioceramic fabrics can help in the treatment of pain and PLM in PPS patients.<br>Dentre as manifestações clínicas da SPP destacam-se nova fraqueza, fadiga, dor, intolerância ao frio, nova atrofia e transtornos do sono. A polissonografia de noite inteira permanece sendo padrão ouro para análise do sono e diagnóstico de transtornos do sono. OBJETIVO: Avaliar o comportamento da dor, intolerância ao frio (IF) e índice de movimentos periódicos de membros (PLMs) após uso de colchonete e roupas com biocerâmica MIG3 por 4 semanas. MÉTODO: 12 pacientes com SPP, da UNIFESP/EPM. Todos realizaram exames de polissonografia e infravermelho e responderam a questionários de dor e IF antes e após o uso dos materiais. RESULTADOS: Houve diminuição significativa da dor e dos PLMs. CONCLUSÃO: Os tecidos com biocerâmica MIG3 podem ser um coadjuvante ao tratamento da dor e dos PLMs nos pacientes com SPP