Tipo de publicación: Sin árbitro

  • Publicación
    Differential efficiency of massive star formation in NGC 628
    The efficiency ratio of massive star formation in the arms of the spiral NGC 628 to that in the interarm region has been determined from the sizes and positions...
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    Diffraction limited imaging in the visible with large ground-based telescopes
    Not Available
  • Publicación
    Diffraction-limited observations of astronomical sources with a rotation shearing interferometer in the near infrared
    An experiment aimed at diffraction-limited imaging of astronomical sources in the 2-5-micron range is presented. It is based on a rotation shearing...
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    Diffractional treatment of curvature sensing in segmented-mirror telescopes
    Discontinuities in the wavefront phase or amplitude affect curvature sensor (CS) response. These discontinuities may be the result of an improper alignment of...
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    Diffuse Emission in the Nucleus of M31
    We will present analysis of the diffuse emission from the nucleus of M31 using a 40 ks Chandra ACIS-S observation. The observation was taken by Chandra on 5...
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    Diffuse gamma-ray line emission from multiple OB associations in Cygnus
    The COMPTEL observations of the diffuse galactic 1.809 MeV emission attributed to the radioactive decay of 26 Al have confirmed the diffuse nature of this...
  • Publicación
    Diffuse gamma-ray line emission from multiple OB Associations in Cygnus
    The COMPTEL observations of the diffuse galactic 1.809 MeV emission attributed to the radioactive decay of 26 Al have confirmed the diffuse nature of this...
  • Publicación
    Diffuse Interstellar Bands in (Proto-) Fullerene-Rich Environments
    The recent infrared detection of fullerenes (C60 and C70) in Planetary Nebulae (PNe) and R Coronae Borealis (RCB) stars offers a beautiful opportunity for...
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    Diffuse Light in Galaxy Groups
    We have studied the amount of diffuse light in two galaxy groups, Leo and HCG 44 through the detection of intragroup planetary nebulae (IGPNe). The emission...