ajtribick wrote:Sorry, either an object is approaching or receding. Relabelling the coordinate axes does not change that. Either one of the stars is closer to us, or the other one is. Again, relabelling the coordinate axes does not change this.
This I have of course never contested!
What I implied, however is illustrated in this little drawing:
If the +z axis points towards the observer and the binary star is travelling towards us (i.e.del > 0) then dz / dt > 0.
If the +z axis points away from the observer and the binary star is travelling towards us then dz / dt < 0.
Sure Celestia (and your script) is off the hook if the convention for radial velocities is such that a positive velocity corresponds to motion towards us.
Yes, i.e. if the +z axis points towards the observer, as I suspect it in Celestia (see drawing!).
I was unable to extract the axis convention for the given radial velocities of that paper. Moreover one always has to separate cleanly between the radial velocity contribution due to orbital movement and movement of the barycenter...I did not see that you've done this cleanly.Can you demonstrate that this is the case - for the four systems I was able to check in the quick test in my previous post (Alpha Centauri, Sigma 2173, 70 Ophiuchi and Chi Draconis) the convention is clearly that the positive velocity corresponds to motion away from us, which means for these systems Celestia is reversed.
Neither there is evidence for the opposite convention in the dominant number of cases where the convention was not specified.There is as yet no evidence that any of the data is using the +ve velocity is towards us convention.
Fridger