Publication type: Refereed

  • Publication
    Polarimetry of Li-rich giants
    Context: .Protoplanetary nebulae typically present non-spherical envelopes. The origin of such geometry is still controversial. There are indications that it...
  • Publication
    Polarimetry of the binary PDS 144
    Aims: Our goal is to study the circumstellar environment associated with each component of the wide intermediate-mass pre-main sequence binary system PDS 144...
  • Publication
    Polarimetry of the transient relativistic jet of GRB 110328/Swift J164449.3+573451
    We present deep infrared (Ks-band) imaging polarimetry and radio (1.4- and 4.8-GHz) polarimetry of the enigmatic transient Swift J164449.3+573451. This source...
  • Publication
    Polarimetry toward the IRAS Vela Shell. I. The Catalog
    We have obtained linear polarization measurements of stars along the western side of the IRAS Vela Shell toward HD 62542. From 16 CCD fields distributed along...
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    Polarimetry toward the IRAS Vela Shell. II. Extinction and Magnetic Fields
    We explore correlations between visual extinction and polarization along the western side of the Infrared Astronomical Satellite (IRAS) Vela Shell using a...
  • Publication
    Polarimetry toward the Musca Dark Cloud. I. The Catalog
    We have used CCD imaging polarimetry to obtain linear polarization measurements of background stars toward the filamentary Musca dark cloud. We present a...
  • Publication
    Polarisation and magnetic fields in cool stars and the Sun. A session in memory of Meir Semel
    Astrophysical plasmas and magnetic fields are inextricably coupled to each other. But magnetic fields are elusive; they cannot be fully characterized with...
  • Publication
    Polarisation du ciel nocturne et polarisation de la lumière zodiacale vers 5000 Å, sur l'ensemble de la sphère céleste
    Not Available
  • Publication
    Polarisation of very-low-mass stars and brown dwarfs. I. VLT/FORS1 optical observations of field ultra-cool dwarfs
    Context: Ultra-cool dwarfs of the L spectral type (T_eff = 1400-2200 K) are known to have dusty atmospheres. Asymmetries of the dwarf surface may arise from...