Tipo de publicación: Sin árbitro

  • Publicación
    A CO Search for Molecular Gas in High Mass Post-Main Nebulae
    Not Available
  • Publicación
    A Combined Analysis of Jeans Kinematics and Milli-Second Pulsar Timing Effects: Probing the Mass Contents of Omega Centauri
    We explore the interplay between Jeans analyses of velocity dispersions and millisecond-pulsar (MSP) timing measurements that trace line-of-sight accelerations...
  • Publicación
    A compact light-weighted and multi-purpose calibration unit for LINC-NIRVANA
    Laboratory and on-sky experience suggests that the integration of big astronomical instruments, specially of a complex interferometric system, is a challenging...
  • Publicación
    A Compact Radio Source Coincident with the Ultraluminous X-Ray Source IC 342 X-1
    We recently discovered an unresolved radio source coincident with the ultraluminous X-ray source (ULX) IC 342 X-1. The radio emission and hard X-ray spectrum of...
  • Publicación
    A Comparative Study of Lithium Abundances, Radial Velocities, and Emission Lines in Pre-Main Sequence Visual Binaries
    Not Available
  • Publicación
    A Comparative Study of the Microvariability Properties in Radio Loud and Radio Quiet Quasars
    We have performed photometric optical observations of a sample of 16 radio loud and 16 radio quiet quasars. The aims were to confirm the existence of...
  • Publicación
    A Comparative Study of the Themis and Veritas Asteroid Families
    Our primary goal is to characterize the surface composition (and other properties such as radius, albedo and thermal inertia) of our sample of Themis-family and...
  • Publicación
    A Comparison of Global Helioseismic-Instrument Performances: Solar-SONG, GOLF and VIRGO
    The SONG spectrograph has recently demonstrated its ability to perform solar radial velocity measurement during the first test run of the Solar-SONG initiative...
  • Publicación
    A Complete Morphological Catalog of Northern Galactic Planetary Nebulae
    Planetary Nebulae (PNe) are highly representative of the last stages of intermediate mass stellar evolution. However, there are still many unresolved questions...