Publication type: Non-refereed

  • Publication
    Close binary central stars and the abundance discrepancy - new extreme objects
    Recent work (Corradi et al. 2015; Jones et al. 2016) has shown that the phenomenon of extreme abundance discrepancies, where recombination line abundances...
  • Publication
    Close Pairs of Lyman Break Galaxies at z 3
    We use a well understood N-body simulation combined with an analytic subhalo model to generate statistics for a defined sample of z 3 Lyman break galaxy (LBG)...
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    Close visual binaries among planetary-mass objects in star-forming regions: the HST view
    Over the past decade, microlensing surveys in field stars and the Gaia-informed census of nearby star-forming regions have convincingly demonsrated the presence...
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    Close-up of primary and secondary asteroseismic CoRoT targets and the ground-based follow-up observations
    To optimise the science results of the asteroseismic part of the CoRoT satellite mission a complementary simultaneous ground-based observational campaign is...
  • Publication
    Closed loop operation with extremely elongated LGS spots in CANARY Phase D
    CANARY is a wide-field AO on-sky test facility which has been operated annually on the 4.2m William Herschel Telescope since 2010. CANARY has the stated goal of...
  • Publication
    Closing in on the launching sites of AGN outflows
    Supermassive black holes, and the outflows they drive, are an established part of our understanding of galaxy evolution. Indeed, cosmological models rely on...
  • Publication
    Cloud phase detection in winter stratiform clouds using Polarimetric Doppler Radar
    Not Available
  • Publication
    Cloudiness and Apparent Rotation Rate of Earth-like Planets
    If we were to observe the light reflected from an extrasolar planet, the portion of the planet reflecting starlight toward us would change due to rotation and...
  • Publication
    Clues to Substellar Formation: Rotation and the Low-Mass End of the Initial Mass Function
    We have monitored S Ori 45, a young, low-mass (20 M j up) brown dwarf of the σ Orionis cluster (˜3 Myr, 352 pc), using optical and near-infrared filters. S Ori...