Pulsar observations using the POLFAR stations

K. Rożko, W. Lewandowski, J. Kijak, A. Krankowski, L. Blaszkiewicz, P. Flisek, K. Chyży, Bartosz Śmierciak
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Abstract

In this paper we present the current status of the pulsar observations conduct by Polish LOFAR stations. In particular we show that the single LOFAR station can provide observations that are of sufficient quality to provide useful scientific data. These can help us to better understand some of the phenomena related to the pulsar emission and the influence of the interstellar matter. In this paper we focus on the mode switching phenomenon and a single pulses analysis conducted for pulsar B0329+54. We find that the same spectral features are visible in both emission modes, so we conclude that the polar cap emission mechanism is the same in separated modes.
使用POLFAR站进行脉冲星观测
本文介绍了波兰LOFAR站脉冲星观测的现状。特别是,我们表明,单个LOFAR站可以提供足够质量的观测,以提供有用的科学数据。这些可以帮助我们更好地理解与脉冲星发射和星际物质影响有关的一些现象。本文主要研究了脉冲星B0329+54的模式切换现象和单脉冲分析。我们发现在两种发射模式下都可以看到相同的光谱特征,因此我们得出结论,在分离模式下,极帽的发射机制是相同的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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