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A&A 442, 97-107 (2005)
DOI: 10.1051/0004-6361:20053325
Polarization microvariability of BL Lacertae objects
I. Andruchow1, 2, G. E. Romero1, 2 and S. A. Cellone21 Instituto Argentino de Radioastronomía, C.C.5, (1894) Villa Elisa, Buenos Aires, Argentina
e-mail: andru@irma.iar.unlp.edu.ar
2 Facultad de Ciencias Astronómicas y Geofísicas UNLP, Paseo del Bosque, B1900FWA La Plata, Argentina
(Received 27 April 2005 / Accepted 10 June 2005)
Abstract
We present the results of a systematic observational
campaign designed to search for microvariability in the optical
polarization of BL Lac objects. We observed a sample formed by 8
X-ray-selected and 10 radio-selected sources, looking for rapid
changes in both the degree of linear polarization and the
corresponding polarization angle. The whole campaign was carried
out during the last three years, and most of the objects were
observed on at least two consecutive nights. The statistical
properties of both classes of BL Lac objects are compared, and
some general conclusions on the nature of the phenomenon are
drawn. In general, radio selected sources seem to display higher
duty cycles for polarimetric microvariability and, on average,
they have a stronger polarization.
Key words: galaxies: active -- galaxies: BL Lacertae objects: general -- polarization
SIMBAD Objects
© ESO 2005
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