Publicaciones

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  • Long-term photometry of IC 348 with the Young Exoplanet Transit Initiative network
    We present long-term photometric observations of the young open cluster IC 348 with a baseline time-scale of 2.4 yr. Our study was conducted with several telescopes from the Young Exoplanet Transit Initiative (YETI) network in the Bessel R band to find periodic variability of young stars. We identified 87 stars in IC 348 to be periodically variable
    Fritzewski, D. J. et al.

    Fecha de publicación:

    11
    2016
    Número de citas
    13
  • Low Resolution Mapping of Comet p/ Halley in the Near Infrared
    We present low resolution maps, of a 4' × 0'.5 region, of comet Halley, in photometric bands J and K, a central scan in the H band and JHKL photometry taken with the 1.5 m Sanchez-Magro Telescope of the Instituto de Astrofisica de Canarias. We obtain central and integrated magnitudes and colours and discuss its variation with distance from the
    Lazaro, C. et al.

    Fecha de publicación:

    11
    1987
    Número de citas
    0
  • Low-mass stars and brown dwarfs in Praesepe
    Presented are the results of a large and deep optical-near-infrared multi-epoch survey of the Praesepe open star cluster using data from the UKIRT Infrared Deep Sky Survey (UKIDSS) Galactic Clusters Survey. Multiple colour-magnitude diagrams were used to select potential members and proper motions were used to assign levels of membership
    Baker, D. E. A. et al.

    Fecha de publicación:

    11
    2010
    Número de citas
    19
  • Low-metallicity (sub-SMC) massive stars
    The double distance and metallicity frontier marked by the SMC has been finally broken with the aid of powerful multi-object spectrographs installed at 8-10m class telescopes. VLT, GTC and Keck have enabled studies of massive stars in dwarf irregular galaxies of the Local Group with poorer metal-content than the SMC. The community is working to
    Garcia, M. et al.

    Fecha de publicación:

    11
    2017
    Número de citas
    11
  • Low-Resolution Maps of Comet p/ Halley in Principal Atomic and Molecular Species
    The authors present maps of a 3arcmin×2arcmin region of the inner coma of comet P/Halley, at 10arcsec resolution, in CN (3883 Å); C2 (5100 Å); C3 (4040 Å); CN (4216 Å); NH2 (6107 Å); [O I] (6300 Å) and CH (4322 Å). The maps were prepared from multi-position absolute spectrophotometry of comet Halley, with 3.6 Å resolution, in the wavelength range
    Kidger, M. R. et al.

    Fecha de publicación:

    11
    1987
    Número de citas
    1
  • Low-resolution spectroscopy and spectral energy distributions of selected sources towards σ Orionis
    Aims: We study in detail nine sources in the direction of the young σ Orionis cluster, which is considered to be a unique site for studying stellar and substellar formation. The nine sources were selected because of their peculiar properties, such as extremely-red infrared colours or excessively strong Hα emission for their blue optical colours
    Caballero, J. A. et al.

    Fecha de publicación:

    11
    2008
    Número de citas
    29