Tipo de publicación: Sin árbitro

  • 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...
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    Very faint X-ray binaries with XMM-Newton
    A population of very faint X-ray binaries has been discovered in the last years thanks to the improvement in sensitivity and resolution of the new generations...
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    Very faint X-ray binaries with XMM-Newton
    A population of very faint X-ray binaries has been discovered in the last years thanks to the improvement in sensitivity and resolution of the new generations...
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    Very First Approach to the Lack of Fast Rotators in Cygnus OB2
    Cygnus OB2, within the Cygnus X complex, is one of the most active star-forming regions of our Galaxy, hosting hundreds of O and B-type stars across different...
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    Very High Energy Observations of PSR B1951+32.
    Not Available
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    Very high energy γ-radiation from the radio quasar 4C 21.35
    A very high energy (VHE) γ-radiation was detected from a flat spectrum radio quasar (FSRQ) 4C 21.35 (PKS1222+21) by MAGIC (Major Atmospheric Gamma Imaging...
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    Very high spatial resolution study of multiplicity in T Tauri systems
    We present first relevant results from our survey to search multiplicity in T Tauri systems and its relation with disk presence and planet formation on these...
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    Very low mass stars and Lithium abundance: the case of UX Tau C
    Not Available
  • Publicación
    Very low mass stars in Praesepe (Boudreault+, 2010)
    The near-infrared (NIR) observations were made on the 3.5m telescope at Calar Alto, Spain (with observation runs of several nights from February 2005 to January...