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Issue A&A
Volume 442, Number 1, October IV 2005
Page(s) 97 - 107
Section Extragalactic astronomy
DOI http://dx.doi.org/10.1051/0004-6361:20053325



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. Cellone2

1  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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