Tipo de publicación: Con árbitro

  • Publicación
    Co-spatial UV-optical HST/STIS spectra of six planetary nebulae: nebular and stellar properties
    This paper represents the conclusion of a project that had two main goals: (1) to investigate to what extent planetary nebulae (PNe) are chemically homogeneous...
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    CO<SUB>2</SUB> as the main parent source of atomic oxygen in comet C/2017 K2 (Pan-STARRS)
    C/2017 K2 (Pan-STARRS) is an Oort cloud comet discovered in May 2017. Ground observations have revealed that this long-period comet was active at heliocentric...
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    COALAS II. Extended molecular gas reservoirs are common in a distant, forming galaxy cluster
    This paper presents the results of 475h of interferometric observations with the Australia Telescope Compact Array towards the Spiderweb protocluster at z=2.16...
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    COALAS. I. ATCA CO(1-0) survey and luminosity function in the Spiderweb protocluster at z = 2.16
    We report a detailed CO(1−0) survey of a galaxy protocluster field at z = 2.16, based on 475 h of observations with the Australia Telescope Compact Array. We...
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    COBRAS: A Space Mission for Mapping the CMB Structure at 0.5° Resolution
    Not Available
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    COBRAS: Goal and Experimental Approach
    Not Available
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    Coherent J/ψ photoproduction in ultra-peripheral PbPb collisions at √{sNN} = 2.76TeV with the CMS experiment
    The cross section for coherent J / ψ photoproduction accompanied by at least one neutron on one side of the interaction point and no neutron activity on the...
  • Publicación
    Coincidence between morphology and star formation activity through cosmic time: the impact of the bulge growth
    The origin of the quenching in galaxies is still highly debated. Different scenarios and processes are proposed. We use multiband (400-1600 nm) bulge-disc...
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    Cold and hot gas distribution around the Milky-Way - M31 system in the HESTIA simulations
    Recent observations have revealed remarkable insights into the gas reservoir in the circumgalactic medium (CGM) of galaxy haloes. In this paper, we characterize...