ANATOMIA, HISTOQUÍMICA E PROSPECÇÃO FITOQUÍMICA DE FOLHAS E RAIZ DE Senna occidentalis (L.) Link e Senna reticulata (Willd.) H. S. IRWIN & BARNEBY USADAS NO TRATAMENTO DE MALÁRIA NA AMAZÔNIA

Malária é uma doença que preocupa as entidades de saúde nos países tropicais pelo número crescente de casos e pela resistência parasitária do protozoário infectante e do mosquito transmissor a inseticidas. Senna occidentalis e S. reticulada são utilizadas no tratamento e profilaxia da malária e o objetivo desse trabalho foi identificar substâncias quimicamente ativas em células e/ou tecidos dessas espécies. Análises anatômicas, histoquímicas e fitoquímicas foram feitas segundo metodologias usuais. As folhas de S. occidentalis e S. reticulata são semelhantes em relação à estrutura anatômica, diferenciando-se na presença de tricomas glandulares em S. occidentalis, papilas na epiderme de S. reticulata, e na composição histoquímica. As raízes das duas espécies analisadas também se assemelham, destacando-se a presença de fibras gelatinosas, cristais prismásticos e drusas. A prospecção fitoquímica revelou cumarinas, flavanonas, catequinas, esteroides livres, saponinas e bases quaternárias

Evidence for Blue Straggler Stars Rejuvenating the Integrated Spectra of Globular Clusters

Integrated spectroscopy is the method of choice for deriving the ages of unresolved stellar systems. However, hot stellar evolutionary stages, such as hot horizontal branch stars and blue straggler stars (BSSs), can affect the integrated ages measured using Balmer lines. Such hot, "non-canonical" stars may lead to overestimations of the temperature of the main sequence turn-off, and therefore underestimations of the integrated age of a stellar population. Using an optimized Hbeta index in conjunction with HST/WFPC2 color-magnitude diagrams (CMDs), we show that Galactic globular clusters exhibit a large scatter in their apparent "spectroscopic" ages, which does not correspond to that in their CMD-derived ages. We find for the first time that the specific frequency of BSSs, defined within the same aperture as the integrated spectra, shows a clear correspondence with Hbeta in the sense that, at fixed metallicity, higher BSS ratios lead to younger "apparent" spectroscopic ages. Thus, the specific frequency of BSSs in globular clusters sets a fundamental limit on the accuracy for which spectroscopic ages can be determined for globular clusters, and maybe for other stellar systems like galaxies. The observational implications of this result are discussed.Comment: 5 pages, 2 figures, 1 table. Accepted for publication in ApJ

Journals’ policies of storage and reuse of raw research data and their impact in five scientific areas

Analisys of journals' policies about storage and re-use of raw research data

Journals’ policies of storage and reuse of raw research data and their impact in five scientific areas

Analisys of journals' policies about storage and re-use of raw research data