Hurst parameter analysis of radio pulsar timing residuals
نویسندگان
چکیده
منابع مشابه
Limits on Planets Orbiting Massive Stars from Radio Pulsar Timing
\Vhen a,massive star collapses to a neutron star, rapidly losing over half its mass in a symmetric supernova explosion, any planets orbiting the star will be unbound. ]Iowever, to explain the observed space velocity and binary fraction of radio pulsars, an asymmetric kick must be given to the neutron star at birth. Occasionally, this kick will prevent the resulting pulsar-planet system from unb...
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ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 2011
ISSN: 0035-8711
DOI: 10.1111/j.1365-2966.2010.18104.x