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by Rebecca Booth0 views·Updated May 16, 2022
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  1. And with the new Polar is absorption spectrum for D
  2. A 5 30 we can get an improved distance estimate.
  3. And given that the previous distance estimate of 2.2 kg parsecs
  4. fell short in predicting the expected characteristics for D A 5 30
  5. We wonder is d.
  6. 530 further away than we thought
  7. with absorption detected from H one at distances past the previous estimate,
  8. we now have evidence that D.
  9. A 5 30 is farther away than we thought.
  10. Now, let's take a closer look at what these two distances can tell us.
  11. Now, let's take
  12. now, let's take a closer look at what these two distances can tell us.
  13. Now, let's take a closer look at what these two distances can tell us about DA 530.
  14. By narrowing down the characteristics of D A 5 30 we are now able
  15. to start to form conclusions about the true distance to the supernova remnant.
  16. Since the 8.3 killer parsecs distance gives unreasonable characteristics for D.
  17. A 5 30. And we are
  18. Since the 8.3 kill a par sec distance gives unreasonable,
  19. Since the 8.3 kill a parsi distance gives unreasonable characteristics for D. A 5 30
  20. and the corresponding absorption at minus 67 kilometers per second.
  21. Can be instead, in Splain by possible association with CTB 102,
  22. We now have an explanation for how the -67 km/s absorption
  23. could actually be related to the 4.44 killer Parsi distance.
  24. And as a result, we're able to start to form the conclusion that D. A 5 30 is A
  25. and as a result, we're able to start to form the conclusion
  26. that D A 5 30 is at the distance of 4.44 killer parsecs,
  27. And we have a new distance measurement to DA 530.