A possible optical counterpart to the old nearby pulsar J0108-1431

Abstract

The multi-wavelength study of old (>100 Myr) radio pulsars holds the key to understanding the long-term evolution of neutron stars, including the advanced stages of neutron star cooling and the evolution of the magnetosphere. Optical/UV observations are particularly useful for such studies because they allow one to explore both thermal and non-thermal emission processes. In particular, studying the optical/UV emission constrains temperature of the bulk of the neutron star surface, too cold to be measured in X-ray observations.Aim of this work is to identify the optical counterpart of the very old (166 Myr) radio pulsar J0108-1431. We have re-analyzed our original VLT observations (Mignani et al. 2003), where a very faint object was tentatively detected close to the radio position, near the edge of a field galaxy. We found that the backward extrapolation of the PSR J0108-1431 proper motion recently measured by CHANDRA(Pavlov et al. 2008) nicely fits the position of this object. Based on that, we propose it as a viable candidate for the optical counterpart to PSR J0108-1431. The object fluxes (U =26.4+/-0.3; B =27.9; V >27.8) are consistent with a thermal spectrum with a brightness temperature of 9X10^4 K (for R = 13 km at a distance of 130 pc), emitted from the bulk of the neutron star surface. New optical observations are required to confirm the optical identification of PSR J0108-1431 and measure its spectrum.

arXiv comment5 pages, 4 figures, submitted to A&A

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• Ultraviolet Emission from the Millisecond Pulsar J0437-4715
• X-ray emission from the old pulsar B0950+08
• Rotochemical Heating in Millisecond Pulsars. Formalism and Non-superfluid case
• X-ray Emission from the nearby PSR B1133+16
• Detection of X-ray Emission from the Very Old Pulsar J0108-1431
• HST Proper Motion confirms the optical identification of the nearby pulsar PSR 1929+10
• The Optical Spectrum of the Vela Pulsar
• Search for the optical counterpart of the nearby pulsar J0108-1431
• Possible optical detection of a fast, nearby radio pulsar PSR B1133+16
• Determination of limits on disc masses around six pulsars at 15 and 90 microns

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