Is PSR B0943+10 a low-mass quark star?
arXiv:astro-ph/0603468 · doi:10.1086/508421
Abstract
A recent X-ray observation has shown that the radio pulsar PSR B0943+10, with clear drifting subpulses, has a much smaller polar cap area than that of conventional pulsars with mass of $\sim\msun$ and radius of km. Zhang et al. (2005) addressed then that this new result conflicts with the standard vacuum gap model. Nonetheless, the discrepancy could be explained if PSR B0943+10 is actually a low-mass quark star. It is found that the potential drop in the open-field-line region of oblique pulsars (i.e., inclination angle ) might be times that of aligned pulsars, and that PSR B0943+10 with could be well above the deathline. We thus conclude that the Ruderman-Sutherland-type vacuum gap model still works well for this pulsar if it is a bare quark star with a mass of and a radius of km.
10 pages, 2 figures, accepted for publication in ApJ Letters
References in corpus (5)
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