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On Sun, 18 Feb 2007 09:31:57 -0000, "George Dishman"
wrote: "Henri Wilson" HW@.... wrote in message .. . On 16 Feb 2007 00:38:58 -0800, "George Dishman" wrote: On 15 Feb, 23:15, HW@....(Henri Wilson) wrote: On 15 Feb 2007 05:33:24 -0800, "George Dishman" wrote: On 15 Feb, 12:48, bz wrote: "George Dishman" wrote oups.com: On 14 Feb, 23:29, bz wrote: HW@....(Henri Wilson) wrote In that case which non-variable spectroscopic binaries have you analysed and what wa the predicted light curve? George, like I said, the biggest problem for me is to find both velocity and brightness curves for the same star. I asked about non-variable stars! "bz" wrote in message . 198.139... The brightness curve looks like this: ---------------------------------------------------- ![]() Brightness curves for near circular orbits are pretty well the same so all I need is the magnitude change and maximum velocity. If you can find some examples for me I will try to match them. You could ask in sci.astro.research, all you need is the velocity curve and a paper that says "No brightness variation has been detected to the level of *** mag." There are plenty of reason why no brightness variation will be expected. There appears to be another factor contributing to light speed unification other than plain space density of matter. Maybe this is related to the gravity field of the stars involved. I have no explanation as yet. Gravity would slightly couteract the speed unification effect but it is a second order effect so increases the unification distance by about one part in ten thousand typically, completely irrelevant as you don't know the distance to within an order of magnitude yet. I'm not trying to explain it at this stage. I just want to find a consistent pattern. Unification distance appears to be definitely related to orbit period. That would suggest a non-linear relation between (v-c/n) and dv/ds. It still needs to be first order at zero but perhaps a third order component? Gravity certainly isn't going to do anything for you. I'm not so sure of that. Well 'rapid' is subjective. What I mean is very much less than the parallax distance to the system. for small period orbits, yes...but not so much for orbits over about a year. Once the light leaves the star, the only remnant of that is the difference between the actual speed and c/n. However the brightness is predicted to go to infinity at the critical distance when the first double image would occur. Since this doesn't seem to happen and multiple images are not commonly observed, I am prepared to accept that exinction rates are normally fairly high. That's all I meant. Typically it must be no more than a fraction of a light year. No. It doesn't work like that. Something makes it period dependent. It can only be the speed. ....and maybe distance between 'pulses'. Similar really. After all, you cannot unify light with other light that hasn't yet been emitted. Nothing of that kind was suggested. The pulsar is an obvious example, each pulse is 45 us or 13.5 km long and they start out 2.95 ms or 885 km apart. The highest frequency shift is 30.54 mHz so over the entire journey, the faster pulses only catch up by 79.7 m. You explained this yourself in another post: "Henri Wilson" HW@.... wrote in message .. . The light from these stars still travels throgh similar quality space, even if it emitted months later. Eventually the pulses change speed (asymptotically as has been said) to c/n but it is the 'quality of space' as you nicely put it that is responsible, not another bunch of photons 885 km away, and bear in mind too that the speed doesn't just come to match adjacent pulses but _all_ the pulses emitted over the 1.5 day orbit end up at exactly the same speed. There's plenty time for that to happen, you figure for the critical distance is 8 light years and the system is over 3000 light years away. there is a lot to be done yet George. George |
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