Tipo de publicación: Con árbitro

  • Publicación
    A new route to graphene starting from heavily ozonized fullerenes: Part 1—thermal reduction under inert atmosphere
    It is shown that heavily ozonized C60 or C70 fullerenes (known also as “fullerene ozopolymers”) are suitable substrates for the preparation of graphene or...
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    A new route to graphene starting from heavily ozonized fullerenes: Part 2—oxidation in air
    Graphite oxide (GO) and heavily ozonized C60 and C70 fullerenes known as “fullerene ozopolymers” were studied by TGA-FTIR (Thermogravimetry coupled with FT-IR...
  • Publicación
    A new route to graphene starting from heavily ozonized fullerenes: Part 3 - an electron spin resonance study
    It is shown that graphite oxide (GO) and both heavily ozonized C60 and C70 fullerenes, known as “fullerene ozopolymers,” are paramagnetic materials with a very...
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    A New sdO+dM Binary with Extreme Eclipses and Reflection Effect
    We report the discovery of a new totally eclipsing binary (R.A. = {06}{{h}}{40}{{m}}{29}{{s}}11; decl. = +38°56‧52″2 J = 2000.0; Rmax = 17.2 mag) with an sdO...
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    A new search for planet transits in NGC 6791
    Context: Searching for planets in open clusters allows us to study the effects of dynamical environment on planet formation and evolution. Aims: Considering the...
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    A new spectroscopic analysis of the massive O + O type binary HD 54662 AB
    HD 54662 AB is one of the three O + OB binaries known so far with orbital period longer than 1000 d, offering the opportunity to test scenarios of massive star...
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    A New Spectroscopic and Photometric Analysis of the Transiting Planet Systems TrES-3 and TrES-4
    We report new spectroscopic and photometric observations of the parent stars of the recently discovered transiting planets TrES-3 and TrES-4. A detailed...
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    A New Spin on Galactic Dust
    We present a new puzzle involving Galactic microwave emission and attempt to resolve it. On one hand, a cross-correlation analysis of the Wisconsin Hα Mapper...
  • Publicación
    A new stellar library in the region of the CO index at 2.3 μm. New index definition and empirical fitting functions
    Context: The analysis of unresolved stellar populations demands evolutionary synthesis models with realistic physical ingredients and extended wavelength...