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Optical photometry of the PSR B0656+14 and its neighborhood

A. B. Koptsevich·G. G. Pavlov·S. V. Zharikov·V. V. Sokolov·Yu. A. Shibanov·V. G. Kurt
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Abstract

We present the results of the broad-band photometry of the nearby middle-aged radio pulsar PSR B0656+14 and its neighborhood obtained with the 6-meter telescope of the SAO RAS and with the Hubble Space Telescope. The broad-band spectral flux $F_ν$ of the pulsar decreases with increasing frequency in the near-IR range and increases with frequency in the near-UV range. The increase towards UV can be naturally interpreted as the Rayleigh-Jeans tail of the soft thermal component of the X-ray spectrum emitted from the surface of the cooling neutron star. Continuation of the power-law component, which dominates in the high-energy tail of the X-ray spectrum, to the IR-optical-UV frequencies is consistent with the observed fluxes. This suggests that the non-thermal pulsar radiation may be of the same origin in a broad frequency range from IR to hard X-rays. We also studied 4 objects detected in the pulsar's 5" neighborhood.

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A. B. Koptsevich, G. G. Pavlov, S. V. Zharikov, V. V. Sokolov, Yu. A. Shibanov, V. G. Kurt. 2000-09-05. Optical photometry of the PSR B0656+14 and its neighborhood. https://doi.org/10.1051/0004-6361%3A20010289

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