Tipo de publicación: Sin árbitro

  • Publicación
    Velocity-Resolved Line Response of the Emission Lines in the High-Luminosity (MV is approximately equal to -24) Seyfert 1 Galaxy Fairall 9
    Not Available
  • Publicación
    Venus Atmospheric Zonal Winds from Contemporaneous Akatsuki UVI and IRTF/SpeX 2.3 µm Images
    We compare Venus dayside cloud top winds from Akatsuki UVI images to contemporaneous winds in the lower clouds retrieved on the night side using IRTF/SpeX 2.3...
  • Publicación
    Venus Cloud Tracking Methods and Applications for Akatsuki, IRTF, and Nordic Optical Telescope Images
    We present cloud-tracking results from Venus nightside images with velocity errors approaching 1 m/s (rms). The cloud-tracking scheme focuses on 1) reducing the...
  • Publicación
    Vertical Stratification of a Sunspot Penumbra
    Not Available
  • Publicación
    Vertical structure of the turbulence above the observatories of the Canary Islands: parameters and statistics for adaptive optics
    The statistics of vertical structure of the turbulence affect the complexity of the design and implementation of Multi-Conjugate Adaptive Optics (MCAO) systems...
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    Vertical Turbulence Profiles at Canary Islands Astronomical Sites
    We present the statistical results of the monitoring of the optical turbulence profiles at the Roque de los Muchachos (ORM) and Teide observatories (OT), Spain...
  • Publicación
    Vertical Velocity Dispersion of the Ionized Gas In NGC 3938
    We have studied the kinematics of the ionized gas in the nearly face-on galaxy NGC 3938 by means of observations made with the Fabry-Perot interferometer TAURUS...
  • Publicación
    Very Efficient Methods for Multilevel Radiative Transfer in Atomic and Molecular Lines
    The development of fast numerical methods for multilevel radiative transfer (RT) applications often leads to important breakthroughs in astrophysics, because...
  • Publicación
    Very energy observations of PSR B1951+32
    PSR B1951+32 is a γ-ray pulsar detected by the Energetic Gamma Ray Experiment Telescope (EGRET) and identified with the 39.5 ms radio pulsar in the supernova...