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On 28 Mar 2007 06:27:41 -0700, "George Dishman"
wrote: On 28 Mar, 11:40, HW@....(Henri Wilson) wrote: On 28 Mar 2007 02:16:59 -0700, "George Dishman" wrote: On 28 Mar, 08:10, HW@....(Henri Wilson) wrote: The diagram would be like this: g h --- O + B The pulsar sends one pulse from g and the next from h, it is orbiting round the barycentre B and the observer is at O. Obviously there is a v*cos(theta) term for other parts of the orbit, it is the distance change in the direction of the line of sight that matters. I have incorporated that by adding an Rsin(x) term to the star distance. It is generally negligible. It will certainly be small but it is not negligible, it will produce a 45 degree phase shift when the ADoppler is about 93 parts per million too and in fact we know that the VDoppler is probably larger than the ADoppler _except_that_ the phase can be changed by the effect you describe at the top of the post regarding an elliptical orbit looking circular. I think I had it right before. The distance for 45 deg phase difference is about 0.0007 LY. It is independent of velocity. "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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