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21.
L. K. N. Cho J. A. Lowe R. B. Maguire J. C. Tsang 《Cellular and molecular life sciences : CMLS》1987,43(4):397-399
Summary Prodigiosin condensing enzyme (PCE) activities were present inSerratia marcescens wild type 08, mutants OF, WF and 9-3-3. Their specific activities exhibited different maxima and at different times during the late log phase or the early stationary phase of cell growth. The levels of prodigiosin and its precursors also showed a significant increase at this period. The results support that prodigiosin and/or its precursors are secondary metabolites. The ubiquity of the PCE activity in mutants deficient in prodigiosin biosynthesis suggest that this particular enzyme may also be present in non-pigmented clinical isolates. 相似文献
22.
Nugent PE Sullivan M Cenko SB Thomas RC Kasen D Howell DA Bersier D Bloom JS Kulkarni SR Kandrashoff MT Filippenko AV Silverman JM Marcy GW Howard AW Isaacson HT Maguire K Suzuki N Tarlton JE Pan YC Bildsten L Fulton BJ Parrent JT Sand D Podsiadlowski P Bianco FB Dilday B Graham ML Lyman J James P Kasliwal MM Law NM Quimby RM Hook IM Walker ES Mazzali P Pian E Ofek EO Gal-Yam A Poznanski D 《Nature》2011,480(7377):344-347
Type Ia supernovae have been used empirically as 'standard candles' to demonstrate the acceleration of the expansion of the Universe even though fundamental details, such as the nature of their progenitor systems and how the stars explode, remain a mystery. There is consensus that a white dwarf star explodes after accreting matter in a binary system, but the secondary body could be anything from a main-sequence star to a red giant, or even another white dwarf. This uncertainty stems from the fact that no recent type Ia supernova has been discovered close enough to Earth to detect the stars before explosion. Here we report early observations of supernova SN 2011fe in the galaxy M101 at a distance from Earth of 6.4 megaparsecs. We find that the exploding star was probably a carbon-oxygen white dwarf, and from the lack of an early shock we conclude that the companion was probably a main-sequence star. Early spectroscopy shows high-velocity oxygen that slows rapidly, on a timescale of hours, and extensive mixing of newly synthesized intermediate-mass elements in the outermost layers of the supernova. A companion paper uses pre-explosion images to rule out luminous red giants and most helium stars as companions to the progenitor. 相似文献