Publication type: Non-refereed

  • Publication
    The contribution to population in ellipticals of blue stragglers - A test of their origin
    An observational test of the binary hypothesis for the origin of the blue straggler (BS) stars has been performed searching for radial velocity variables among...
  • Publication
    The control unit of the near infrared spectrograph of the Euclid space mission: detailed design
    The Near Infrared Spectrograph and Photometer (NISP) is one of the instruments on board the ESA EUCLID mission. The Universidad Poli&tacute;ecnica de Cartagena...
  • Publication
    The control unit of the near infrared spectrograph of the EUCLID space mission: preliminary design
    The Near Infrared Spectrograph and Photometer (NISP) is one of the instruments on board the ESA EUCLID mission. The Universidad Politecnica de Cartagena and...
  • Publication
    The cool neutral phase of the local ISM: compact clouds carry a major fraction of the mass
    Not Available
  • Publication
    The cooling tail of a long X-ray burst from XTE J1701-407
    Swift XRT observed the recently discovered source XTE J1701-407 (Markwardt et al., ATel #1569, Degenaar et al., ATel #1572) on July 17th, 2008 at UT 13:31:45...
  • Publication
    The coordinated key role of wet, mixed, and dry major mergers in the buildup of massive early-type galaxies at z < 1
    Hierarchical models predict that massive early-type galaxies (mETGs) derive from the most massive and violent merging sequences occurred in the Universe...
  • Publication
    The COrE+ (Cosmic Origins Explorer) mission
    COrE+ has been proposed to ESA as a medium-class mission for investigating, within the framework of the ESA Cosmic Vision program, a set of important scientific...
  • Publication
    The Coronae of AB Dor and V471 Tau: Youth vs Tidal Spin-Up
    We report on an analysis of high resolution Chandra spectra of two stars with very similar spectral types and rotation rates but with very different...
  • Publication
    The Coronal Line Spectrum of the Brightest Seyfert Galaxies as Seen by ISO
    The ISO coronal line spectrum of a sample of the brightest known Seyfert galaxies is presented and modeled. ISO observations of [O IV] 25.9 μ, [Ne V] 14.3 μ,...