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2012•Astronomy and AstrophysicsOpen access

Possible optical counterpart of PSR J1357−6429

A. Danilenko, A. Yu. Kirichenko, R. E. Mennickent, George G. Pavlov, Yu. A. Shibanov, S. V. Zharikov, D. A. Zyuzin

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Abstract

Context. PSR J1357−6429 is a Vela-like radio pulsar that has been recently detected in X-rays and γ-rays. It powers a compact tail-like X-ray pulsar wind nebula and X-ray-radio plerion associated with an extended TeV source HESS J1356−645.

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What this paper is about

Context. PSR J1357−6429 is a Vela-like radio pulsar that has been recently detected in X-rays and γ-rays. It powers a compact tail-like X-ray pulsar wind nebula and X-ray-radio plerion associated with an extended TeV source HESS J1356−645.

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Available abstract

Context. PSR J1357−6429 is a Vela-like radio pulsar that has been recently detected in X-rays and γ-rays. It powers a compact tail-like X-ray pulsar wind nebula and X-ray-radio plerion associated with an extended TeV source HESS J1356−645.

Key concepts: Pulsar, Physics, Astrophysics, Pulsar wind nebula, Pulsar planet, Vela, Nebula, Binary pulsar

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