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On 25 Mar 2007 05:54:00 -0700, "Jerry" wrote:
On Mar 25, 2:41 am, "Jerry" wrote: This is not to say that the surface of the white dwarf companion of PSR J1909-3744 is non-turbulent. Far from it. Tidal effects from the closely orbiting pulsar would be expected to drive complex "weather" patterns on its surface. That, of course, is assuming that the white dwarf is not in a state of tidal lock, with one face always directed towards the pulsar. Even so, the gradual cooling of the white dwarf should drive convective effects. Stellar surfaces are not quiescent, even on dead stars. However, any luminosity variances due to these effects would be completely negligible relative to the flux of black body radiation. There could, of course, be minor variations due to the white dwarf not being entirely spherical due to tidal distortion, etc. theories, theories.....all based on completely wrong interpretations of basic data. Jerry "When a true genius appears in the world, you may know him by this sign, that the dunces are all in confederacy against him." --Jonathan Swift. |
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