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Monthly Notices of the Royal Astronomical Society, Vol. 414, Iss. 2, 2011-06 ,pp. : 992-1010

Oxford University Press

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Origin of pulsars with 0.1_S < P < 0.3_S and 5 × 10⁵ years < τ < 10⁷ years after the second supernova explosion in high-mass X-ray binaries

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Astronomical and Astrophysical Transactions, Vol. 23, Iss. 5, 2004-10 ,pp. : 497-498

Taylor & Francis Ltd

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Origin of pulsars with 0.1 s < P < 0.3 s and 5 × 10⁵ years < τ < 10⁷ years after the second supernova explosion in high-mass X-ray binaries

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Comparison of GONG and MDI solar p-mode background

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Solar Physics, Vol. 220, Iss. 2, 2004-04 ,pp. : 399-402

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The influence of a finite conductivity on the spectrum of solar p-modes

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