Please use this identifier to cite or link to this item: http://hdl.handle.net/1959.3/55891
- Title
- Simultaneous single-pulse observations of radio pulsars II. Orthogonal polarization modes in PSR B1133+16
- Author(s)
-
Karastergiou, A.;
Kramer, M.;
Johnston, S.;
Lyne, A. G.;
Bhat, N. D. R.;
Gupta, Y.
- Abstract
- In this letter, we present a study of orthogonal polarization modes in the radio emission of PSR B1133+16, conducted within the frame of simultaneous, multi-frequency, single-pulse observations. Simultaneously observing at two frequencies (1.41 GHz and 4.85 GHz) provides the means to study the bandwidth of polarization features such as the polarization position angle. We find two main results. First, that there is a high degree of correlation between the polarization modes at the two frequencies. Secondly, the modes occur more equally and the fractional linear polarization decreases towards higher frequencies. We discuss this frequency evolution and propose propagation effects in the pulsar magnetosphere as its origin.
- Publication type
- Journal article
- Source
-
Astronomy and Astrophysics,
Vol. 391, no. 1 (Aug 2002), pp. 247-251
- Publication year
- 2002
- FOR Code(s)
-
0201 Astronomical and Space Sciences
- Keyword(s)
-
Pulsars;
PSR B1133+16
- Publisher
- EDP Sciences
- ISSN
- 0004-6361
- Publisher URL
- http://dx.doi.org/10.1051/0004-6361:20020793
- Copyright
- Copyright © 2002 ESO. The published version is reproduced in accordance with the copyright policy of the publisher.
- Full text

- Peer reviewed
