Publication type: Non-refereed

  • Publication
    Boxy/Peanut bulges and stellar bars
    Boxy/peanut bulges in disc galaxies have been associated to stellar bars. We analyse their properties in a large sample of $N$-body simulations, using different...
  • Publication
    Boxy/peanut bulges, vertical buckling and galactic bars
    Boxy/peanut bulges in disk galaxies have been associated to stellar bars. In this talk, we discuss the different properties of such bulges and their relation...
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    Break type and interactions from ultra-deep optical imaging of isolated galaxies
    In the standard cosmological model of galaxy evolution, mergers and interactions play a fundamental role in shaping galaxies. Galaxies that are currently...
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    Breaks and truncations: a unified picture for spiral galaxies
    Departures from a simple exponential decay (usually called breaks or truncations) in the surface brightness distribution of galaxy disks are found in the vast...
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    Bright galaxies from the WENSS minisurvey (de Ruiter+ 1998)
    A search for bright galaxies associated with radio sources from the Westerbork Northern Sky Survey (WENSS) minisurvey has been carried out. A galaxy counterpart...
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    Bright galaxies in 5 medium redshift clusters. I. (Ascaso+, 2008)
    Two of us (M.M. and J.A.L.A.) imaged five galaxy clusters with the 2.5m Nordic Optical Telescope (NOT) located at the Roque de Los Muchachos Observatory (La...
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    Bright mid-infrared detections of MAXI J1836-194 with VISIR on the VLT: brightening of the compact jet
    The new X-ray transient MAXI J1836-194 is a black hole candidate X-ray binary (BHXB; ATel #3611, #3613, #3628 #3652). Its X-ray spectrum was seen to soften...
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    Bright Young Star Clusters in NGC5253 with LEGUS
    Using UV-to-H broad and narrow-band HST imaging, we derive the ages and masses of the 11 brightest star clusters in the dwarf galaxy NGC5253. This galaxy...
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    Brightening of WZ Sge
    We report on a sudden brightening of the dwarf nova WZ Sge during decline from outburst (cf. IAUC #7669, IAUC #7670). The observations were made with the 0.82-m...