Eumicetoma de grãos pretos por Madurella grisea: registro de dois casos Eumycotic mycetoma of black grains caused by Madurella grisea: report of two cases

Os Autores registram dois casos de eumicetoma de grãos pretos, com localização podal, procedentes da Bahia, provocados por Madurella grisea Mackinnon et al., 1949. São estudadas a estrutura dos grãos, bem como as características micromorfológicas do fungo em vida saprofítica. Acreditam os Autores que estas observações correspondem ao sétimo e oitavo casos registrados na literatura do país, provocadas por este fungo. Os Autores consideram nomen dubium ou nomina confusa as seguintes espécies de Madurella: M. ramiroi, M. oswaldoi, M. bovoi, M. tozeuri, M. mansonii, M. brumpti, M. reynieri, M. americana, M. lackawanna e M. ikedae, o mesmo ocorrendo com a chamada Rubromadurella mycetomi. As únicas espécies válidas são Madurella mycetomatis McGinnis, 1980 (=Madurella mycetomi Brumpt, 1905) e Madurella grisea Mackinnon et al., 1949. Nos dois casos registrados o tratamento com itraconazol, por um período de 3 meses não fez regredir as lesões, havendo ligeira melhora clínica.<br>Two cases of black grains eumycotic mycetoma, occurring on a foot, are reported. Both proceeded from the State of Bahia (Brazil), and in both the etiologic agent was Madurella grisea Mackinnon et al., 1949. The grains structure as well as the micromorphologic characteristics of the fungus in saprophytic life were studied. It is the Author's belief that these observations correspond to the 7th and 8th cases reported in the Brazilian medical literature. The Authors do consider the following Madurella species as nomen dubium or nomina confusa: M. ramiroi, M. oswaldoi, M. bovoi, M. tozeuri, M. mansonii, M. brumpti, M. reynieri, M. americana, M. lackawanna e M. ikedae and the same for Rubromadurella mycetomi. The only valid species must be Madurella mycetomatis McGinnis, 1980 (=Madurella mycetomi Brumpt, 1905) and Madurella grisea Mackinnon et al., 1949. Treatment with itraconazole in both reported cases, for a 3 month duration, did not produce any regression of the lesions, the clinical improvement being meager

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