Zobrazeno 1 - 10
of 21
pro vyhledávání: '"Jaroslaw Dyks"'
Autor:
Shunshun Cao, Jinchen Jiang, Jaroslaw Dyks, Longfei Hao, Kejia Lee, Zhixuan Li, Jiguang Lu, Zhichen Pan, Weiyang Wang, Zhengli Wang, Jiangwei Xu, Heng Xu, Renxin Xu
Publikováno v:
The Astrophysical Journal, Vol 973, Iss 1, p 56 (2024)
As one of the paradigm examples to probe into pulsar magnetospheric dynamics, PSR B0943+10 (J0946+0951) manifests representatively, showing a mode switch, orthogonal polarization, and subpulse drifting, frequently studied below 600 MHz. Here, both in
Externí odkaz:
https://doaj.org/article/7bcc9d7246e746bfb98b88dd64bdd01f
Autor:
Jaroslaw Dyks
Single pulse behaviour of radio pulsars is usually interpreted in terms of the ExB drift of a radio beam. It is shown that antisymmetric arrangement of the radio-bright zones can produce several types of observed single pulse phenomena: the half-cycl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::225a6b68513a30b91c20a3d216bc26af
http://arxiv.org/abs/2203.05572
http://arxiv.org/abs/2203.05572
Autor:
Jaroslaw Dyks, Bronislaw Rudak
Publikováno v:
Proceedings of 7th International Fermi Symposium — PoS(IFS2017).
The pulsed radiation from PSR B0833-45 (Vela) has a phased-averaged spectral energy distribution of an apparently simple structure across a wide energy range. However, in narrow energy bands the pulses reveal astonishing complexity of the directional
Autor:
Jaroslaw Dyks, Bronislaw Rudak
Publikováno v:
Proceedings of the International Astronomical Union. 8:301-306
Highly symmetric double features observed in averaged pulsar profiles can be interpreted as the imprint of microscopic radiation beam characteristic of radiative mechanism operating in pulsar magnetosphere. The data put strong constraints on the poss
Autor:
Shiho Kobayashi, David N. Burrows, Peter Mészáros, Neil Gehrels, Yi-Zhong Fan, Bing Zhang, John A. Nousek, Jaroslaw Dyks
Publikováno v:
The Astrophysical Journal. 642:354-370
(Abridged) The Swift X-Ray Telescope (XRT) reveals some interesting features of early X-ray afterglows, including a distinct rapidly decaying component preceding the conventional afterglow component in many sources, a shallow decay component before t
Autor:
Alice K. Harding, Jaroslaw Dyks
Publikováno v:
The Astrophysical Journal. 614:869-880
We study the rotational distortions of the vacuum dipole magnetic field in the context of geometrical models of the radio emission from pulsars. We find that at low altitudes the rotation deflects the local direction of the magnetic field by at most
Publikováno v:
The Astrophysical Journal. 606:1125-1142
We present the influence of the special relativistic effects of aberration and light travel time delay on pulsar high-energy lightcurves and polarization characteristics predicted by three models: the two-pole caustic model, the outer gap model, and
Autor:
Jaroslaw Dyks, B. Rudak
Publikováno v:
The Astrophysical Journal. 598:1201-1206
We present a new model of high-energy lightcurves from rotation powered pulsars. The key ingredient of the model is the gap region (i.e. the region where particle acceleration is taking place and high-energy photons originate) which satisfies the fol
Autor:
Jaroslaw Dyks, Bronislaw Rudak
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 319:477-483
Autor:
Jaroslaw Dyks, Bronislaw Rudak
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 295:337-343
We present a modified scenario of gamma-ray emission from pulsars within the framework of polar cap models. Our model incorporates possible acceleration of electron-positron pairs created in magnetospheres, and their subsequent contribution to gamma-