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Träfflista för sökning "WFRF:(Pasquali A) srt2:(2010-2014)"

Sökning: WFRF:(Pasquali A) > (2010-2014)

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  • Christodoulou, C., et al. (författare)
  • Tuning the work function of graphene-on-quartz with a high weight molecular acceptor
  • 2014
  • Ingår i: The Journal of Physical Chemistry C. - : American Chemical Society (ACS). - 1932-7447 .- 1932-7455. ; 118:9, s. 4784-4790
  • Tidskriftsartikel (refereegranskat)abstract
    • Ultraviolet and X-ray photoelectron spectroscopies in combination with density functional theory (DFT) calculations were used to study the change in the work function (Φ) of graphene, supported by quartz, as induced by adsorption of hexaazatriphenylene-hexacarbonitrile (HATCN). Near edge X-ray absorption fine structure spectroscopy (NEXAFS) and DFT modeling show that a molecular-density-dependent reorientation of HATCN from a planar to a vertically inclined adsorption geometry occurs upon increasing surface coverage. This, in conjunction with the orientation-dependent magnitude of the interface dipole, allows one to explain the evolution of graphene Φ from 4.5 eV up to 5.7 eV, rendering the molecularly modified graphene-on-quartz a highly suitable hole injection electrode. 
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3.
  • Wu, S. -W, et al. (författare)
  • The discovery of a very massive star in W49
  • 2014
  • Ingår i: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 568, s. L13-
  • Tidskriftsartikel (refereegranskat)abstract
    • Context. Very massive stars (M > 100 M-circle dot) are very rare objects, but have a strong influence on their environment. The formation of this kind of objects is of prime importance in star formation, but observationally still poorly constrained. Aims. We report on the identification of a very massive star in the central cluster of the star forming region W49. Methods. We investigate near infrared K-band spectroscopic observations of W49 from VLT/ISAAC together with JHK images obtained with NTT/SOFI and LBT/LUCI. We derive the spectral type of W49nrl, the brightest star in the dense core of the central cluster of W49. Results. On the basis of its K-band spectrum, W49nrl is classified as an O2-3.5If* star with a K-band absolute magnitude of -6.27 +/- 0.10 mag. The effective temperature and bolometric correction are estimated from stars of similar spectral type. After comparison to the Geneva evolutionary models, we find an initial mass between 100 M-circle dot and 180 M-circle dot. Varying the extinction law results in a larger initial mass range of 90-250 M-circle dot
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  • Resultat 1-5 av 5

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