Astrometric Measurements and Proper Motion Analysis for WDS 11582 +0335 HJ 1204
Abstract
We obtained and analyzed CCD images of the double star system WDS 11582 +0335 (HJ 1204) using the iTelescope network and a variety of specialized software. WCS coordinates were attached to each image, and the separation distance (ρ) and mean position angle (θ) were measured at ρ = 7.9" ± 0.03" and θ = 59.3° ± 0.2°. These results were compared to historical data, dating back 200 years and we find that HJ 1204 is currently exhibiting a linearly decreasing ρ and a constant θ. This suggests that HJ 1204 could be a visual double or an edge-on binary. Follow-up spectroscopic observations should resolve the two possibilities.
- Publication:
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Journal of Double Star Observations
- Pub Date:
- April 2018
- Bibcode:
- 2018JDSO...14..334E